This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU
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,2461146.6518,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.1522+42.9089,2461146.6518,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J086.1522+42.9089 20260416.1518 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 J082.5944+47.6498,2461146.6518,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.5944+47.6498 20260416.1518 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055127.94+451129.9,2461146.6518,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J055127.94+451129.9 20260416.1518 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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,2461146.6518,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
ASASSN-V J055339.78+470552.3,2461146.6518,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J055339.78+470552.3 20260416.1518 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
target,2461146.6518,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
Gaia DR3 962016844026504832,2461146.6518,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962016844026504832 20260416.1518 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197964319802625792,2461146.6518,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197964319802625792 20260416.1518 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 J086.8513+48.1175,2461146.6518,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.8513+48.1175 20260416.1518 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962640125385001856,2461146.6518,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962640125385001856 20260416.1518 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967581128777104000,2461146.6518,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967581128777104000 20260416.1518 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
target,2461146.6518,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 J084.6295+48.7004,2461146.6518,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6295+48.7004 20260416.1518 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 208280796888874240,2461146.6518,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208280796888874240 20260416.1518 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 J082.0152+49.4731,2461146.6518,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0152+49.4731 20260416.1518 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 J083.2285+44.1845,2461146.6518,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.2285+44.1845 20260416.1518 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.6414+46.2737,2461146.6518,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J079.6414+46.2737 20260416.1518 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
target,2461146.6518,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
ATO J092.3424+49.4237,2461146.6518,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J092.3424+49.4237 20260416.1518 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.8851+48.3378,2461146.6518,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J087.8851+48.3378 20260416.1518 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2879+46.2213,2461146.6518,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J089.2879+46.2213 20260416.1518 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3456+46.8139,2461146.6518,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.3456+46.8139 20260416.1518 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461146.6518,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208934456550670592 20260416.1518 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963599002602153728,2461146.6518,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963599002602153728 20260416.1518 11.76CV 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 J090.7252+43.4870,2461146.6518,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J090.7252+43.4870 20260416.1518 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196564783236506368,2461146.6518,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 11.80CV 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 J085.0114+50.0334,2461146.6518,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J085.0114+50.0334 20260416.1518 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 214356977317828864,2461146.6518,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214356977317828864 20260416.1518 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7984+46.2495,2461146.6518,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J087.7984+46.2495 20260416.1518 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197968717848571264,2461146.6518,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197968717848571264 20260416.1518 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194505775916838272,2461146.6518,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194505775916838272 20260416.1518 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196143842081588352,2461146.6518,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196143842081588352 20260416.1518 12.21CV 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 J087.0101+43.3293,2461146.6518,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J087.0101+43.3293 20260416.1518 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211566141928805888,2461146.6518,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211566141928805888 20260416.1518 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212655861031529216,2461146.6518,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212655861031529216 20260416.1518 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
target,2461146.6518,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196796848908972032,2461146.6518,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208055504381217280,2461146.6518,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208055504381217280 20260416.1518 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3861+47.5396,2461146.6518,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J090.3861+47.5396 20260416.1518 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 J082.0489+43.4659,2461146.6518,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0489+43.4659 20260416.1518 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9292+49.3005,2461146.6518,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J088.9292+49.3005 20260416.1518 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209704634383239936,2461146.6518,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209704634383239936 20260416.1518 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 J084.9230+50.9576,2461146.6518,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.9230+50.9576 20260416.1518 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207620613173739776,2461146.6518,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207620613173739776 20260416.1518 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 J084.3627+42.0135,2461146.6518,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.3627+42.0135 20260416.1518 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461146.6518,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.1639+48.2580,2461146.6518,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.1639+48.2580 20260416.1518 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461146.6518,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.2234+48.7629,2461146.6518,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.2234+48.7629 20260416.1518 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461146.6518,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 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
ZTF J051728.60+465934.4,2461146.6518,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J051728.60+465934.4 20260416.1518 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461146.6518,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 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
target,2461146.6518,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212612842640667008,2461146.6518,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212612842640667008 20260416.1518 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8834+47.5321,2461146.6518,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8834+47.5321 20260416.1518 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
target,2461146.6518,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 J083.5567+44.2856,2461146.6518,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5567+44.2856 20260416.1518 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,2461146.6518,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461146.6518,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052927.90+475833.1,2461146.6518,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J052927.90+475833.1 20260416.1518 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
target,2461146.6518,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 J083.5805+44.4532,2461146.6518,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5805+44.4532 20260416.1518 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
ATO J084.8541+42.6555,2461146.6518,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.8541+42.6555 20260416.1518 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461146.6518,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.1629+50.0440 20260416.1518 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 J091.0747+46.9169,2461146.6518,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.0747+46.9169 20260416.1518 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 J089.5381+48.6224,2461146.6518,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3038+45.6310,2461146.6518,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.3038+45.6310 20260416.1518 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212372114013974528,2461146.6518,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212372114013974528 20260416.1518 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970027988825374592,2461146.6518,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970027988825374592 20260416.1518 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970478994751036800,2461146.6518,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970478994751036800 20260416.1518 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210142480528630656,2461146.6518,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210142480528630656 20260416.1518 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053001.72+474541.1,2461146.6518,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J053001.72+474541.1 20260416.1518 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.7520+48.5869,2461146.6518,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J080.7520+48.5869 20260416.1518 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6873+48.2843,2461146.6518,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212980796780702848,2461146.6518,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212980796780702848 20260416.1518 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197161641956644864,2461146.6518,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197161641956644864 20260416.1518 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.8530+42.8735,2461146.6518,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.8530+42.8735 20260416.1518 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 J088.6178+44.7898,2461146.6518,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J088.6178+44.7898 20260416.1518 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210459483474791296,2461146.6518,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210459483474791296 20260416.1518 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970601104965241472,2461146.6518,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970601104965241472 20260416.1518 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 963318524057490944,2461146.6518,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963318524057490944 20260416.1518 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 J092.3958+50.3918,2461146.6518,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J092.3958+50.3918 20260416.1518 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
Gaia DR3 197183292886359680,2461146.6518,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053745.20+455814.5,2461146.6518,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1518 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 214238642379208832,2461146.6518,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214238642379208832 20260416.1518 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207305495716713344,2461146.6518,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207305495716713344 20260416.1518 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2615+46.3117,2461146.6518,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J088.2615+46.3117 20260416.1518 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.9565+45.0681,2461146.6518,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J086.9565+45.0681 20260416.1518 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 J094.1293+46.6157,2461146.6518,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J094.1293+46.6157 20260416.1518 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8999+48.2678,2461146.6518,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.8999+48.2678 20260416.1518 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.1530+42.8276,2461146.6518,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.1530+42.8276 20260416.1518 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 J091.3234+48.2792,2461146.6518,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.3234+48.2792 20260416.1518 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 211249448220214656,2461146.6518,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1518 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197871479789423488,2461146.6518,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197871479789423488 20260416.1518 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.0214+42.2947,2461146.6518,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J080.0214+42.2947 20260416.1518 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3650+48.6832,2461146.6518,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.3650+48.6832 20260416.1518 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
target,2461146.6518,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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 194352153525496320,2461146.6518,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194352153525496320 20260416.1518 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.5288+48.9426,2461146.6518,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J086.5288+48.9426 20260416.1518 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.5230+44.0250,2461146.6518,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J092.5230+44.0250 20260416.1518 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6206+45.0339,2461146.6518,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.6206+45.0339 20260416.1518 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
Gaia DR3 960777247745760640,2461146.6518,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 960777247745760640 20260416.1518 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J064853.3+491958,2461146.6518,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J064853.3+491958 20260416.1518 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5685+50.2412,2461146.6518,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5685+50.2412 20260416.1518 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
ATO J085.0615+41.5382,2461146.6518,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J085.0615+41.5382 20260416.1518 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.5705+42.4844,2461146.6518,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.5705+42.4844 20260416.1518 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.1563+47.3181,2461146.6518,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J097.1563+47.3181 20260416.1518 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197321075438633984,2461146.6518,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197321075438633984 20260416.1518 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962395282184785152,2461146.6518,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962395282184785152 20260416.1518 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[EHV2002] 1-3-0242,2461146.6518,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
[EHV2002] 1-3-0242 20260416.1518 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.0690+42.7256,2461146.6518,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.0690+42.7256 20260416.1518 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209407731883788928,2461146.6518,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209407731883788928 20260416.1518 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963132809671621504,2461146.6518,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963132809671621504 20260416.1518 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 J089.8999+48.2678,2461146.6518,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.8999+48.2678 20260416.1518 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7204+41.4088,2461146.6518,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7204+41.4088 20260416.1518 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962055872391939584,2461146.6518,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962055872391939584 20260416.1518 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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
ATO J096.1811+43.5089,2461146.6518,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J096.1811+43.5089 20260416.1518 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.6832+48.4651,2461146.6518,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.6832+48.4651 20260416.1518 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
ASASSN-V J053730.29+442702.5,2461146.6518,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J053730.29+442702.5 20260416.1518 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 214474895644533376,2461146.6518,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214474895644533376 20260416.1518 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.8612+47.4654,2461146.6518,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J090.8612+47.4654 20260416.1518 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.7810+41.1861,2461146.6518,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J090.7810+41.1861 20260416.1518 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.6179+43.5583,2461146.6518,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J088.6179+43.5583 20260416.1518 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210478862367382784,2461146.6518,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210478862367382784 20260416.1518 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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,2461146.6518,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193139186041201280,2461146.6518,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193139186041201280 20260416.1518 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.98CV 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
target,2461146.6518,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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,2461146.6518,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.8478+50.4009,2461146.6518,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.8478+50.4009 20260416.1518 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,2461146.6518,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.5553+49.0572,2461146.6518,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.5553+49.0572 20260416.1518 14.10CV 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 J084.2052+41.6684,2461146.6518,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.2052+41.6684 20260416.1518 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.4611+47.5880,2461146.6518,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J088.4611+47.5880 20260416.1518 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963647484194177408,2461146.6518,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963647484194177408 20260416.1518 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208033136192150528,2461146.6518,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208033136192150528 20260416.1518 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,2461146.6518,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6518,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 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,2461146.6518,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1518 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VY Aur,2461146.6518,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VY Aur 20260416.1518 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461146.65216699 16.04.2026 03:38:57.228 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
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: 10 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): 23472
Objects passed selection criteria: 23461
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 21980.8
Average stars matched: 21486.8 (97.7526 %)
Memory usage VmPeak: 126876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:46:48 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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461146.65216699 16.04.2026 03:38:57.228 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 577
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 186 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): 169528
Objects passed selection criteria: 169113
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 161414
Average stars matched: 155554 (96.3697 %)
Memory usage VmPeak: 1941560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:51:59 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.65137969
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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:13.103 +45:58:37.04 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 06:00:13.103 +45:58:37.04
Angular distance between the image centers 0.0803 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:10.737 +45:58:56.46 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 06:00:10.737 +45:58:56.46
Angular distance between the image centers 0.0718 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 06:00:13.103 +45:58:37.04
Second-epoch second image center 06:00:10.737 +45:58:56.46
Angular distance between the image centers 0.00872 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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.wyhpSiHJ85
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.ylvfsM7suW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits &> /tmp/tmp.nDNue92UaE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits &> /tmp/tmp.diewxIUckP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_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 23 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
15.2 mag. fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
15.2 mag. fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.wyhpSiHJ85 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_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-Q1b1x1_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.ylvfsM7suW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_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-Q1b1x1_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.nDNue92UaE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1626, passed=19987
Got 19987 stars (including 18331 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat
util/solve_plate_with_UCAC5 got 19987 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.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.diewxIUckP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1539, passed=19937
Got 19937 stars (including 18372 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat
util/solve_plate_with_UCAC5 got 19937 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 19458 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 19458 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 19458 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31756.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31503_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31503_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:19.02 +41:59:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 2.748 195128614893796992 079.82981792246 +41.98936411498 12.6943 12.1849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31505_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31505_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:17.41 +45:15:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.138 207978912228439680 083.57253136688 +45.25065668779 12.3739 12.0939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31551_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31551_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:27.48 +44:52:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 0.989 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31561_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31561_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:14:59.12 +46:47:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31573_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31573_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:59:43.41 +44:59:10.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31580_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31580_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:27.61 +42:19:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 0.645 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31586_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31586_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:37:23.01 +46:49:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.244 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31593_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31593_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:42.22 +43:22:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31650_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31650_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:45:42.91 +43:37:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31676_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31676_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:17:36.71 +45:34:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.411 962542440648583424 094.40310292280 +45.56864166395 12.1582 11.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31682_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31682_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:38:21.21 +50:18:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31699_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31699_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:46:04.80 +47:26:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.219 966672004459585152 101.51999576409 +47.43461621313 12.0973 11.3733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31701_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31701_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:06:11.33 +47:25:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.836 969681535286381312 091.54712051726 +47.42216425873 12.0045 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31703_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31703_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:14:23.61 +46:49:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.310 968668648856984832 093.59826702611 +46.82539996683 12.0731 11.3523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31704_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31704_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:20.90 +43:16:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.785 193310160099657216 088.83737940998 +43.28199553885 12.1323 11.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31708_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31708_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:31.23 +42:40:34.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31723_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31723_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:05:57.47 +43:47:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.500 961201758017019648 091.48936574688 +43.78965603324 12.2410 11.5458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31729_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31729_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:23.99 +48:22:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31743_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31743_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:12:35.14 +45:58:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.318 962606074882449920 093.14648896912 +45.96717746347 12.0488 11.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:17:51.95 +46:05:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.804 968565496626029440 094.46613657377 +46.08352223629 12.3932 12.0762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31756_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 31756_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:56.84 +42:44:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.288 192496212256963072 089.48694131592 +42.74832301273 12.3100 11.9498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:01.83 +50:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:41:12.80 +44:09:59.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Aur-02-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:13.103 +45:58:37.04 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 06:00:13.103 +45:58:37.04
Angular distance between the image centers 0.0803 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:10.737 +45:58:56.46 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 06:00:10.737 +45:58:56.46
Angular distance between the image centers 0.0718 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 06:00:13.103 +45:58:37.04
Second-epoch second image center 06:00:10.737 +45:58:56.46
Angular distance between the image centers 0.00872 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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.qOUDppanH4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.sVWDglqsJ4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits &> /tmp/tmp.YdGB6DqTM7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits &> /tmp/tmp.8QwbpDtHYo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_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.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 546 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.3 mag. fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
14.3 mag. fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.6 (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.qOUDppanH4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_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-Q1b1x1_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.sVWDglqsJ4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_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=51, blended=20075, passed=170053
Got 170053 stars (including 149705 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170053 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166991 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(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_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-Q1b1x1_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.YdGB6DqTM7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=15006, passed=154984
Got 154984 stars (including 139725 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat
util/solve_plate_with_UCAC5 got 154984 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 39.8 to 51.4)
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: 938 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 151620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 39.8 to 51.4)
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: 938 matched stars entering correct_measured_positions(), 151619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 151619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.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.8QwbpDtHYo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=14681, passed=153237
Got 153237 stars (including 138333 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat
util/solve_plate_with_UCAC5 got 153237 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 39.8 to 51.4)
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: 936 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 150094 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 39.8 to 51.4)
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: 936 matched stars entering correct_measured_positions(), 150094 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 150093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.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-Q1b1x1_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_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_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_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-37-49_20.00sec_-4.90C_LIGHTs_0072.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q1b1x1_224001_TTUQ1b1x1_7427_sPwX16tU/wcs_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out195332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68332.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 271s
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: 169s
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Considering the candidate 195316_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195316_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:56.74 +46:03:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.280 208828495415485952 080.48644220986 +46.05425590073 14.4023 13.4470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195322_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195322_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:53.16 +43:34:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.571 207589895567588224 079.97135351461 +43.57410440585 14.2930 13.3348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195332_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195332_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:46.42 +42:34:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.998 194686370700914176 084.19336771424 +42.57383043954 14.6898 13.8832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195340_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195340_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195346_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195346_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:38.29 +46:28:16.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195354_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195354_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:55.03 +42:47:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.525 195440326440226816 081.73024686227 +42.78905799049 14.5721 13.9691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195360_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195360_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:17.33 +42:15:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.615 192412473278709376 088.82312410410 +42.25231695679 14.4947 13.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195368_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195368_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195372_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195372_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:37.02 +47:19:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.841 198072316756880128 089.40458914425 +47.33015345967 14.7107 13.9246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195374_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195374_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:25.69 +50:40:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.106 211636167075334784 089.35780735602 +50.66645121652 14.7329 14.0571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195379_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195379_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:09:32.92 +41:55:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.517 960595862686503168 092.38749783264 +41.92849142401 14.6920 14.0093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195383_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195383_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:36.07 +50:36:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.519 211624759642265728 088.65051018604 +50.61021009047 14.6311 14.0005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195384_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195384_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195386_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195386_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195390_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195390_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:52.03 +45:30:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.847 208563650552312448 080.46729016708 +45.51273702823 14.2343 13.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195405_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195405_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:15.00 +45:31:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.222 196920402231000832 089.06263104547 +45.51793777272 14.3071 13.6688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195410_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:59.37 +49:26:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.899 211286694176443648 089.24755543055 +49.44861273434 14.4035 13.8229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195414_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195414_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195421_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195421_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:58.01 +50:10:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.565 215062722046343040 083.99189946912 +50.16926274295 14.3623 13.5648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195422_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195422_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:23.55 +44:44:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195426_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195426_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:24.25 +50:20:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.042 211569852780732288 089.35236411573 +50.33418129791 14.5141 13.8996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195429_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195429_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195432_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195432_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:50.68 +41:07:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195434_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:13:59.85 +49:18:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.724 969387351503471104 093.49968336657 +49.30775203185 14.4278 13.9576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195438_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195438_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:21.45 +50:13:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.875 213771040699836928 081.08956308169 +50.22245562380 14.2097 13.3039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195439_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195439_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:29.21 +50:48:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.568 214608142708363904 087.62182050965 +50.80269248900 14.4520 13.7482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195447_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195447_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:08.44 +41:15:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.436 194930324844149632 081.03600089012 +41.25802378144 14.2178 13.3555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195448_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195448_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:27.47 +43:48:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.706 195611163059241088 083.61450272044 +43.80372310162 14.1797 13.5453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195449_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195449_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195450_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195450_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:21.71 +50:53:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.241 214639513150353024 088.84073309163 +50.88659093024 14.5161 13.9710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195455_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195455_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:04.13 +50:05:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.654 211551161082978432 088.51749029006 +50.09856694290 14.2592 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195461_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195461_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:36.43 +48:19:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195467_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195467_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:52.10 +51:08:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.593 215361278110871296 083.71690410243 +51.13657417348 14.3956 13.5541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195469_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195469_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:01:01.98 +48:38:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.487 969814580490083584 090.25833473206 +48.64796014011 14.3056 13.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195472_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195472_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:27.88 +46:36:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.534 211869572780914176 080.11602646961 +46.61493983045 14.3131 13.7478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195473_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195473_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195478_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:04:41.78 +42:52:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195479_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195479_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:30.87 +43:18:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.461 195573195548727936 082.87914012941 +43.30520585144 14.1180 13.1690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195483_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:03:36.81 +47:42:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.110 969703667255081728 090.90347088593 +47.71592073831 14.4357 13.8490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195484_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195484_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:45.72 +45:03:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.527 208070485227164928 081.94101142153 +45.06080533679 13.8936 13.0276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195485_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195485_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:49.78 +44:48:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.198 208040248657612928 081.70764333414 +44.80979192182 14.1883 13.6321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195486_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195486_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:34.81 +50:07:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195487_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195487_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:15:21.92 +51:00:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.149 262515277377693184 078.84127118194 +51.00031902678 13.8897 13.3600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195491_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195491_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:22:09.11 +50:01:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:41:26.77 +43:07:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195506_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195506_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:21.18 +41:17:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195507_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195507_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:15.76 +49:01:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195513_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195513_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:31.42 +50:29:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.597 213829898932109312 082.88161004974 +50.48582548102 14.2748 13.4673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195515_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195515_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195517_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195517_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195524_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195524_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:33.03 +42:15:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195525_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195525_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:31.73 +42:04:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195530_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195530_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:29.66 +46:12:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.560 209537817853642752 085.12292055667 +46.20279066372 14.1709 13.3563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195535_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195535_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:57.71 +42:35:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195541_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195541_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:53.14 +43:23:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195546_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195546_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:10.24 +43:55:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195548_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195548_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:18:26.33 +43:29:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195550_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195550_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:46.63 +47:09:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195555_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195555_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:11:03.90 +44:42:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195563_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:31.29 +42:08:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.409 195038111342984832 081.38049763012 +42.14459603839 14.0228 13.5076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195565_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195565_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:46.27 +48:52:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195567_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195567_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:41.83 +49:49:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.266 211307825415448192 089.42481236490 +49.82328526168 13.9006 13.0749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195581_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195581_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:37:43.75 +50:23:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195583_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195583_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:08.76 +49:41:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195584_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195584_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:53.96 +47:59:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195585_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195585_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:18.80 +41:20:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195587_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195587_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:56.99 +48:15:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.034 210349291794699776 087.48789679493 +48.25673838420 13.6819 13.0962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195592_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195592_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:59.28 +46:26:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.287 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195593_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195593_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:52.49 +46:29:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195594_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195594_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:35.78 +48:01:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.449 212371289380254336 081.89926390564 +48.01699616597 13.7292 13.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:15:57.52 +41:11:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195599_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195599_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:59.54 +44:37:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.841 207708127426423808 080.74876747824 +44.62546209328 13.6319 12.8108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195600_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195600_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:50.72 +41:27:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195602_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195602_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:18.40 +47:51:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195603_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195603_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:08.03 +41:09:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195605_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195605_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:44.43 +43:14:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195606_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195606_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:31.95 +41:33:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195608_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195608_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195609_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195609_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:44.20 +50:59:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.670 215225007387998592 085.93446186108 +50.98390711228 13.5660 12.9195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195610_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195610_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:55.63 +50:56:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195611_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195611_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195614_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195614_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195616_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195616_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:53.36 +43:56:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195619_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195619_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195621_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195621_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:50.77 +49:51:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195622_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195622_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:16:42.98 +44:42:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.913 962379987803965568 094.17937221668 +44.71614908613 13.4420 12.7072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195624_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195624_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:50.43 +44:24:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195626_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195626_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:28:02.52 +42:27:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195627_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195627_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:16:36.27 +44:32:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.671 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195632_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195632_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:21.97 +42:50:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195635_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195635_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195637_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195637_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195640_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195640_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:00.13 +43:23:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195641_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195641_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:01.72 +46:28:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.901 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195642_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195642_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:51.28 +41:14:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.817 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195643_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195643_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:19:25.25 +44:38:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195647_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195647_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:01:39.53 +45:44:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.859 963145561432116224 090.41445434671 +45.73787381455 13.0287 12.5054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195649_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195649_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:24.74 +42:28:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195650_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195650_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:47.68 +43:12:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195651_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195651_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:37:03.06 +42:12:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195653_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195653_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:37.07 +41:20:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195654_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195654_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:23.64 +49:53:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195656_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195656_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:14.20 +42:05:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:00:34.59 +45:32:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.699 963062342146066432 090.14422902412 +45.53343101528 12.7393 12.0346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195658_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195658_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195659_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195659_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:24.85 +41:49:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.222 192332281946142720 087.60399164976 +41.81961455802 12.4764 11.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195661_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195661_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:45.97 +43:34:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195662_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195662_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195663_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195663_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:48:07.45 +45:19:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.238 197617561323923584 087.03135150238 +45.31853933119 12.1463 11.6118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195664_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195664_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:42.53 +41:42:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195666_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195666_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:54.74 +41:11:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.02, MAG_FAINT_SEARCH_LIMIT=11.00)GAIADR2_OUTPUT=# 1.876 195065736570175232 079.47860479966 +41.19823177411 10.9555 10.7152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195738_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195738_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195742_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195742_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:27.58 +42:19:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.10, MAG_FAINT_SEARCH_LIMIT=11.08)GAIADR2_OUTPUT=# 0.525 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195746_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195746_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:42.21 +43:22:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:44:52.56 +49:21:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195809_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195809_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195851_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195851_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:11:34.57 +48:44:35.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195852_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195852_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:48.08 +43:44:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195868_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195868_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195899_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195899_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:01.47 +41:06:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195901_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:31.42 +50:41:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.152 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195907_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195907_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:38.35 +45:26:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195925_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195925_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:46:26.57 +47:55:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.106 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195946_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195946_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 195949_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 195949_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:06:21.38 +48:46:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.828 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 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#
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Considering the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196015_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196015_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196026_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196026_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:39:07.56 +44:53:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.057 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196029_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196029_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196040_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196040_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196046_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196046_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:37.57 +45:55:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196049_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196049_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:51.84 +42:57:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196053_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196053_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196068_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196068_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:05:50.20 +44:39:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.514 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196093_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196093_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:09.66 +47:19:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.732 212316245079377280 081.04053074053 +47.31751152611 12.7573 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196097_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196097_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196099_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196099_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:40.90 +44:01:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.561 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196101_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196101_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196112_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196112_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:43.95 +41:06:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196124_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196124_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:02.42 +49:49:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.675 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196135_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196135_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196136_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196136_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196152_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196152_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196165_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196165_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:25.96 +48:47:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196170_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196170_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:41:16.81 +47:26:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.074 210685257018537344 085.32032670455 +47.44841135014 13.1638 12.3736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196176_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196176_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196178_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196178_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:30:40.67 +41:28:15.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196185_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196185_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:56.73 +46:08:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196186_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196186_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:12:10.21 +50:14:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196197_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196197_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:03:13.61 +42:56:27.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196205_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196205_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:31.99 +45:54:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196210_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196210_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:16.18 +46:04:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.457 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196247_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196247_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:28:43.93 +42:26:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196261_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196261_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:12.03 +45:24:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.637 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 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#
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Considering the candidate 196266_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196266_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:46:42.70 +50:56:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196268_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196268_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:45.34 +50:03:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.484 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196283_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196283_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:51.79 +41:10:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196286_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196286_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:06.76 +46:10:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196300_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196300_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:15.10 +40:57:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196306_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196306_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:01:04.66 +50:00:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.250 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196318_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196318_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196330_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196330_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:17.71 +42:18:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196336_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196336_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:30:09.29 +46:12:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.083 209019462542689408 082.53951456145 +46.21579217952 13.5370 12.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:59.37 +46:40:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196371_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196371_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:13:42.17 +45:31:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196379_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196379_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196383_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196383_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:17.81 +43:17:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196387_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196387_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:51.27 +48:55:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.471 210461201461752192 089.21406534870 +48.93146143301 13.6447 13.0132 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#
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Considering the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196401_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196401_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:03.63 +46:04:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196402_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196402_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196413_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196413_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:14.27 +50:00:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196419_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196419_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:52:03.69 +49:32:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196422_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196422_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:36.03 +45:44:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196425_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196425_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:01.97 +42:43:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.041 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196428_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:54.09 +43:54:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196429_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196429_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196436_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196436_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196444_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196444_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:10:01.87 +47:39:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.197 969468887162852736 092.50786637866 +47.65128419673 13.7413 13.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196450_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196450_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:24.02 +43:46:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.380 195777429833427968 083.35022209389 +43.77985576823 13.6692 12.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196460_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196460_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:44.83 +44:40:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.880 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196462_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196462_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:51.21 +46:21:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196466_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196466_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:00:13.97 +47:43:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.401 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196485_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196485_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:41.51 +50:41:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.480 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196486_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196486_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196487_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196487_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:38.68 +41:49:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196489_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:30.35 +41:38:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196502_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196502_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:57.50 +43:06:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.250 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196503_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196503_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:41.19 +48:21:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196512_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196512_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:27.56 +46:35:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196532_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196532_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196534_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196534_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196535_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196535_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:40.36 +42:51:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196536_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196536_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196541_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196541_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:05.65 +48:44:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196542_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196542_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:28:50.57 +44:16:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196547_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196547_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:38.87 +43:41:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196557_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196557_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:06.27 +45:12:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196559_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:47.37 +47:00:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.678 212303050943149440 080.69756548932 +47.01475255644 13.7614 13.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196560_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196560_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:30.33 +43:50:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.621 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196561_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196561_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:02.50 +46:44:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196565_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196565_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:02.97 +49:04:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196566_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196566_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:46.10 +41:46:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196568_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196568_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:59:21.25 +45:06:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.572 196674081564004352 089.83869973985 +45.11475185016 13.8009 13.0282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196576_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196576_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196586_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196586_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:49.10 +51:04:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:40.74 +41:24:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196604_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196604_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:38:50.45 +49:49:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196613_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196613_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196616_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196616_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:46:39.80 +43:21:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196618_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196618_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:45.78 +44:42:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196628_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196628_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:52:21.19 +42:50:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196638_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196638_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:45.48 +45:22:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196639_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196639_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:29.08 +49:47:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196646_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196646_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:08:21.85 +42:58:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:18.24 +46:15:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196663_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196663_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:24.82 +49:14:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196667_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196667_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:31.38 +42:59:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196670_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196670_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:17.29 +45:05:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196671_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196671_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:48:07.71 +50:26:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.550 214568598946171264 087.03234717596 +50.43577947810 13.9372 13.3806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196675_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196675_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196676_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196676_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:34:28.00 +50:19:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196681_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196681_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:13.42 +46:47:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196690_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196690_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:28.95 +46:52:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.952 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196698_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196698_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:50.77 +48:07:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.490 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196705_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196705_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:51:57.05 +41:37:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.867 192277649962098688 087.98771623166 +41.62337032686 13.8897 13.1157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196708_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196708_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:07.99 +42:49:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.191 194739697014485760 083.53365490341 +42.81724823285 14.0507 13.1567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196714_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196714_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:18.67 +47:12:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.066 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196716_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196716_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:24.79 +44:48:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.101 208086290707268608 081.10372106703 +44.80994290569 13.9169 13.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196717_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196717_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:08.59 +50:16:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196722_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196722_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:48:44.70 +49:34:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.486 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196728_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196728_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:28.64 +41:25:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196729_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196729_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:23:09.76 +49:10:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.823 970593653198168064 095.79099454777 +49.16629137386 14.1385 13.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196732_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196732_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:27.83 +47:51:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196740_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196740_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:41.24 +44:16:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196744_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196744_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196746_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196746_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:39:15.60 +45:20:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196751_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196751_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196755_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196755_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:28:49.59 +49:26:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196761_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196761_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:00.72 +49:05:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.962 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196764_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196764_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:03:43.68 +50:12:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196781_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196781_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:23:43.16 +50:10:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.562 213769219633738112 080.92960190688 +50.17639561905 13.7633 12.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196789_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196789_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:37:44.75 +42:36:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.210 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196794_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196794_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:04.97 +42:33:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196795_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196795_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:18:35.26 +46:39:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196796_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196796_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:52:55.13 +42:18:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196800_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196800_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196802_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196802_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196810_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196810_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:44.13 +47:47:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.196 212218358483551616 079.93457606840 +47.79294561915 13.8506 12.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196811_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196811_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:11:51.76 +45:03:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.484 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196825_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196825_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:16.23 +43:16:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.529 196045745028719488 085.56775371942 +43.27358583012 14.0728 13.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196828_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196828_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:34.15 +46:53:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196830_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196830_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:11.27 +42:50:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.922 192511364902195840 089.29695470380 +42.84027162771 14.0339 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196836_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196836_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:18.44 +46:56:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196837_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196837_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196843_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196843_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:58.71 +46:09:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196845_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196845_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:12:20.00 +50:12:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.283 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196853_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196853_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196856_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196856_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196868_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196868_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196869_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196869_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:52:59.19 +46:57:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196878_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196878_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196880_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196880_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:29.89 +49:54:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.541 971091731965538688 096.62459838265 +49.90271527912 14.1099 13.5701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196884_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196884_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:37.53 +42:21:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196889_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196889_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196891_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196891_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196896_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196896_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:23:48.59 +48:50:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196913_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196913_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:12:44.95 +47:30:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.538 968792721871861888 093.18747696802 +47.51186298846 14.0070 13.4569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196924_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196924_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:38:59.92 +47:35:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.965 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196926_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196926_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:45:24.76 +43:50:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196930_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196930_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:56.85 +44:02:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196934_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196934_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196938_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196938_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:04:15.56 +42:17:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196947_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196947_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196948_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196948_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196951_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196951_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:53.94 +46:32:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.087 209184908981247744 081.97518253378 +46.54961465738 14.0914 13.2181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196952_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196952_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:00.74 +46:20:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.173 208287501334038656 083.50390290064 +46.33909529807 14.0153 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196970_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196970_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:07.21 +47:47:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.393 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196978_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196978_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:42.32 +49:50:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196984_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196984_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:09.12 +45:30:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.203 208175935264007040 082.78821481371 +45.51453490536 14.1469 13.5285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196986_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196986_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:10:13.62 +49:41:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.569 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196993_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196993_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196997_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196997_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:31.26 +41:51:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196998_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 196998_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 196999_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 196999_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:09:10.27 +42:04:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197007_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197007_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197011_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197011_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197015_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197015_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:21.39 +42:12:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.797 194485228791887360 083.83941947095 +42.21584423136 13.9826 12.9019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197016_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197016_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197019_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197019_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:56.34 +50:48:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.754 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197021_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197021_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:24.04 +41:41:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197033_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197033_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:36.13 +44:09:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197042_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197042_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:06.48 +46:08:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197077_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197077_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197084_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197084_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197103_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197103_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:10.87 +46:03:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.092 197523351216767360 086.79557643499 +46.05504755708 14.1430 13.2999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197109_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197109_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:52.99 +45:11:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197110_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197110_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197116_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197116_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:09.10 +50:39:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.101 213847353679179392 082.78816156270 +50.65301417970 14.2713 13.7490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197119_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197119_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:29:34.09 +51:10:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.408 261966208758451968 082.39187092852 +51.16684242895 14.0311 13.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197147_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197147_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197150_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197150_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197154_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197154_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:41.62 +49:06:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197155_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197155_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:12.67 +49:24:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197170_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197170_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197188_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197188_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:41.87 +43:20:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.573 195519044600902912 083.42618984021 +43.33514083335 14.2551 13.3080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197190_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197190_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:47.88 +46:19:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197200_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197200_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197202_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197202_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197207_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197207_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:47.38 +45:58:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197218_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197218_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197219_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197219_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:41:40.25 +42:55:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197223_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197223_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197232_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197232_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:39:33.88 +49:48:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.959 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197237_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197237_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197242_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197242_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197254_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197254_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:21.43 +42:55:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.970 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197276_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197276_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197288_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197288_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:33.69 +42:33:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197306_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197306_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:13.35 +43:49:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.680 196352989809398528 085.80547782617 +43.82085122128 14.3638 13.9452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197314_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197314_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197318_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197318_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:41:07.45 +47:58:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197325_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197325_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:10:00.22 +45:32:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.629 963235820168851712 092.50109436752 +45.54496087176 14.4482 13.9808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197336_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197336_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197340_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197340_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197345_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197345_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197364_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197364_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:28:08.51 +47:14:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.019 209275275092603648 082.03571968964 +47.24927946107 14.4467 13.5625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197370_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197370_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:41.44 +44:10:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.677 208347699597359744 079.17292871064 +44.17938943448 14.3058 13.4443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197375_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197375_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197389_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197389_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197403_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197403_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:27.24 +41:03:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.390 194265704424465536 083.61355838690 +41.05137680810 14.3213 13.5068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197409_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197409_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:08:51.54 +44:11:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197423_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197423_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197424_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197424_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:54.17 +42:18:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.547 195184002791881344 079.97609641765 +42.30073591294 14.4162 13.8720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197436_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197436_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:54.42 +50:17:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.501 261848144399968512 079.97690685320 +50.29554219310 14.5876 13.9065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197458_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197458_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197459_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197459_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:55.36 +47:16:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197465_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197465_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:36.63 +50:11:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.905 215075473806779008 083.90235443786 +50.19653993164 14.3478 13.7275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197470_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197470_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:17.31 +47:02:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197478_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197478_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197482_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197482_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197483_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197483_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197484_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197484_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:18:04.38 +42:31:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197504_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197504_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:04.04 +43:45:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.157 195601336173976832 084.01706491764 +43.76183674387 14.2172 13.4494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197521_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197521_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197522_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197522_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197526_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197526_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197532_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197532_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:22.62 +45:21:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.360 207994550205149568 083.34478647209 +45.35922558133 14.6379 14.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197543_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197543_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197545_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197548_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197548_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197549_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197549_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:51:07.98 +44:47:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197553_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197553_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197558_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197558_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:07.96 +49:17:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.212 213659199752081152 080.28295225740 +49.28554282609 14.5830 13.7560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197574_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197574_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:44:46.85 +46:28:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.194 209612206687131136 086.19689831834 +46.47272458834 14.4861 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197588_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197588_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197589_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197589_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:44:45.58 +43:08:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.720 196074779007819520 086.19014372164 +43.13658694549 14.6415 13.7929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197598_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:25.77 +48:41:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.333 212507220802710016 083.35834626956 +48.68617781390 14.7540 14.0993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197610_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197610_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 197618_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197618_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:38.60 +44:09:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.656 207786055312951808 081.91124517927 +44.15132482194 14.4460 13.8037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197634_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197634_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:36.15 +44:35:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.012 195891950840782848 083.65111377781 +44.59892370072 14.6504 14.0523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197657_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:24.77 +47:49:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.765 212549380203108736 081.35368248338 +47.81982154758 14.5991 13.8771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197660_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197660_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197666_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197666_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197670_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197670_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:02:55.88 +43:20:58.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197673_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197673_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197674_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197674_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:51:17.42 +48:38:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.615 210393066101070976 087.82317447496 +48.64291830688 14.5406 13.7761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197680_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197680_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:46.20 +49:43:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.431 970717073378527488 096.44268224399 +49.72986681373 14.6980 14.1083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197688_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197688_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:24.94 +42:29:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.371 195432320621288832 081.60363280080 +42.49773498546 14.3030 13.3587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197695_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197695_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197699_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197699_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197702_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197702_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197711_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197711_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197716_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197716_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:20:26.81 +50:46:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197721_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197721_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:24.74 +43:20:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.944 207387271893470592 080.35360583400 +43.34019971885 14.5582 13.7955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197722_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197722_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:04.73 +46:46:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.589 211875001618915840 080.51925488235 +46.77557355019 14.2946 13.4026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197724_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197724_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:25:22.39 +44:07:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.860 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197730_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197730_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:48.84 +47:50:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.381 210849603944817664 083.95385514517 +47.83981062777 14.4444 13.5806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197742_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197742_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197748_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:31:49.72 +49:27:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.668 968009663434056576 097.95727002455 +49.45668034899 14.7177 14.1135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197760_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197760_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197761_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197761_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197762_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197762_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:03:02.74 +46:43:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.639 963597151473005312 090.76167548963 +46.73289191284 14.4883 13.8730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197772_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197772_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:08:13.04 +41:54:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197779_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197779_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:04.43 +48:09:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.336 212995266527595136 079.76873019899 +48.16487078047 14.6081 13.7325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197785_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197785_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197797_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197797_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:54:16.12 +41:58:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.125 192299846352802176 088.56714256474 +41.96732700967 14.4620 13.6806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197801_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197801_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:12.45 +46:37:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.185 211860707967806848 080.55175356227 +46.62856539187 14.2153 13.3047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197807_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197807_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:41:34.67 +49:47:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.988 991170807152733952 100.39442081091 +49.79644893955 14.8011 14.2964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197819_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197819_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:59:51.36 +51:05:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.621 211664376420455168 089.96466731365 +51.09810907484 14.6737 14.0602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197836_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197836_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:42.98 +50:45:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.828 261920441587057920 081.67937594654 +50.76503030054 14.5633 13.9408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197838_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197838_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197840_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197840_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197846_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197846_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:29:36.66 +48:08:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.189 212457845858919424 082.40318324799 +48.13661800230 14.5949 14.0236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197847_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197847_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:43:51.92 +41:39:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.766 192757792945027968 085.96660850387 +41.66113921297 14.5630 13.9268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197849_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197849_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197854_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197854_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:46:01.47 +49:53:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.749 991219254384148992 101.50644388813 +49.89019966890 14.4079 13.6620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197860_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197860_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197863_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197863_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197869_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197869_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:24.18 +50:46:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.522 214773314267550336 086.85082920768 +50.76666959922 14.8342 14.2774 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#
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Considering the candidate 197890_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197890_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:43:45.71 +49:57:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.550 991141326497157888 100.94030652244 +49.94980277396 14.7648 14.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197891_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197891_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197892_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197892_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:42:27.33 +49:57:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.593 991185856718109568 100.61419868533 +49.95083816550 14.8624 14.3736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197900_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197900_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197901_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197901_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197913_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197913_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197917_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197917_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:36:53.02 +41:42:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.365 957893052650528000 099.22104953821 +41.70818806157 14.8478 14.3270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197920_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197920_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:47.35 +50:09:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.609 213617349589966336 083.19727919748 +50.15836353964 14.8015 14.1412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197923_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197923_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:20:58.65 +48:14:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.614 212987295068205568 080.24457466648 +48.23522639915 14.6451 13.8292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197932_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197932_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:30:45.87 +50:35:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.996 213840550451010560 082.69152597529 +50.58630810280 14.7089 13.8690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197935_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197935_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:17:58.14 +47:16:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.274 968738708363404416 094.49176873886 +47.27147482170 14.8875 14.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197941_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197941_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197942_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197942_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:14.13 +45:07:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.165 208539388279559936 080.30930540676 +45.13275868881 14.3732 13.5291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197949_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197949_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197954_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197954_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197957_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 197957_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 197960_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197960_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:17:16.76 +47:13:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.300 212165994242529280 079.31971235374 +47.22607009996 14.7276 13.9714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197967_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197967_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:36:03.28 +50:26:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.225 215081933437508480 084.01375296660 +50.44158093136 14.7920 14.0329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197971_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197971_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:02:02.85 +41:50:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.141 960759896078081536 090.51141856402 +41.84365110628 14.7475 14.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197974_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197974_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:29:42.85 +46:33:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.485 209085231379835904 082.42899258963 +46.55253351000 14.7077 14.1466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197978_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197978_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:23:07.46 +41:42:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.404 194955854129646976 080.78155453086 +41.70269254078 14.7420 14.2496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197990_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197990_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:01:32.48 +48:06:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.505 969772008774566528 090.38550220391 +48.10359754765 14.5671 13.9081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197992_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 197992_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:50:53.90 +41:48:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.784 192330220361813248 087.72459655970 +41.80447694898 14.5853 14.0080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198010_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198010_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198018_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198018_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:11:19.24 +49:00:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.937 970024999528133120 092.82999804225 +49.01001446715 14.8171 14.1270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198021_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198021_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:30:20.00 +41:45:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.450 194542987512991360 082.58340667026 +41.75869331153 14.4203 13.5063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198023_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198023_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198026_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198026_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:34:10.10 +41:40:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.326 194438190310265984 083.54224606777 +41.67970776656 14.7136 14.1641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198040_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198040_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198045_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198045_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:33.71 +50:11:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.719 215118182961669120 083.39110593441 +50.19559635934 14.6762 14.0761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198046_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198046_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:50.55 +41:11:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.186 194282094019283328 083.46141177934 +41.18408814875 14.5582 13.8420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198048_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198048_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:37:20.50 +50:18:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.532 991950154739160192 099.33558822426 +50.31674458895 14.7249 14.1994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198050_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198050_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:52:47.14 +44:31:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.930 196585467798665600 088.19677367178 +44.52709383905 14.7170 14.1455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198059_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:41:14.15 +50:06:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.923 991200184728965632 100.30870735959 +50.10051842780 14.8162 14.2502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198060_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198060_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198061_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198061_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:08:47.21 +50:16:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.475 971727623346464512 092.19672769043 +50.28304808655 14.5608 13.8694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198067_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198067_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:30:07.52 +47:57:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198071_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198071_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198074_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198074_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 198080_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198080_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:10:00.33 +46:40:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.274 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198084_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198084_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:03.92 +50:06:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.021 214366696828682624 085.01667763881 +50.10168318636 14.7297 13.9311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198087_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198087_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198094_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198094_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:23:59.23 +46:05:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.739 209155703203888640 080.99675522363 +46.09812834135 14.1555 13.1152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198101_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198101_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198113_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198113_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:55:38.44 +43:35:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.496 193335105269222016 088.91091577639 +43.59165155998 14.6568 13.8803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198114_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198114_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198118_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198118_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:23.58 +50:30:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.464 215132717130829440 083.84815980346 +50.50527351684 14.8350 13.9632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198130_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198130_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:23.68 +48:57:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.452 967664554221753856 096.59862735180 +48.96326598147 14.7320 14.1364 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#
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Considering the candidate 198135_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198135_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198137_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198137_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:11:54.42 +50:05:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.456 971666226790759936 092.97691490727 +50.09027042044 14.7153 14.0031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198140_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198140_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:02.10 +48:58:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.647 213639683420721664 080.25896026909 +48.97063878089 14.5755 13.7510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198144_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198144_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198146_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198146_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:56.31 +50:34:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.372 215142711518296448 083.48484082941 +50.57531109403 14.6845 13.8592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198148_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198148_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:26:04.63 +45:47:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.702 208937450145275648 081.51969485534 +45.79671145051 14.9540 14.4643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198149_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198149_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:57.13 +45:47:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.575 208937347066066560 081.48862920288 +45.79890361237 14.5349 13.6442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198151_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198151_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:39:04.98 +50:07:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.068 214323510932539648 084.77096721916 +50.12648801163 14.8238 14.2123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198154_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198154_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198157_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198157_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198158_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198158_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:02.40 +46:25:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.677 209168759903993216 081.25987560660 +46.42951446126 14.5931 13.6562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198162_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198162_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198166_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198166_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198169_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198169_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:44:27.03 +50:33:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.973 214403225525499648 086.11220251936 +50.56264222298 14.7783 14.1780 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#
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Considering the candidate 198171_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198171_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:56:51.71 +45:34:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.065 196921025003426304 089.21565386917 +45.58232105393 14.8705 14.3501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198172_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198172_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:29:41.76 +51:06:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.867 261953907972120832 082.42478555200 +51.11582723483 14.6486 14.0220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198174_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198174_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:13:35.50 +49:52:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.750 970909724135187072 093.39804852101 +49.88177354060 14.8975 14.1967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198175_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198175_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198176_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198176_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:02:30.63 +50:59:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.336 972007900029519232 090.62783787004 +50.98809849152 14.7042 14.0186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198183_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198183_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:14.60 +45:19:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.226 208158411797493632 082.81090972626 +45.33124508497 14.6953 14.0907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198184_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198184_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:35:40.15 +50:06:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.354 215062348386740992 083.91782718919 +50.11434658747 14.7441 13.9320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198206_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198206_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198208_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198208_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:45.48 +48:24:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.315 210974879549224704 085.69014813049 +48.41418871241 14.9400 14.2309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198210_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198210_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:19:24.38 +50:22:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.665 261861067958266112 079.85089832061 +50.36998686505 14.6430 13.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198218_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198218_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198223_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198223_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198224_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198224_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:32:27.95 +41:13:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.996 194326486801321472 083.11700206516 +41.23115324650 14.5458 14.0984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198228_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198228_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:12.46 +44:49:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.387 207943384257399808 082.80204930430 +44.82926529385 14.6480 13.9019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198234_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198234_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198238_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198238_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:44:28.39 +42:31:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.270 193031674419463808 086.11877011634 +42.51971519176 14.4802 13.6125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198239_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198239_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:56.32 +43:42:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.895 207560655429828864 079.23453363343 +43.70604854565 14.6081 13.7298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198243_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198243_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:38:17.76 +42:30:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.165 195984447255724672 084.57394327643 +42.51407404908 14.7207 14.1108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198246_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:33:50.32 +49:02:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.598 214206859621359616 083.45968022942 +49.03797310049 14.7767 14.1647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198248_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198248_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:16:26.33 +48:13:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.224 213028148796886656 079.11015542728 +48.22619180815 14.5601 13.9150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198250_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198250_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:48:19.66 +44:14:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.155 196751116097754112 087.08236455430 +44.24330025787 14.7193 13.8907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198255_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198255_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:39:18.82 +46:40:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.164 209759575604369920 084.82861277952 +46.67351168016 14.8166 14.1638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198256_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198256_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198261_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198261_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:49:29.07 +42:28:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.392 193169113373091712 087.37164333181 +42.46913586159 14.6077 13.7720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198264_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198264_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198266_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198266_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198269_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198269_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:31:01.97 +49:15:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.848 212779315571030144 082.75844249681 +49.26102946891 14.8899 14.2412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198272_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198272_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198281_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198281_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:22:21.16 +46:30:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 3.241 211856275562094080 080.58791339020 +46.51428339890 14.6686 13.8413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198298_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198298_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:53:16.19 +41:27:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.695 192095440268927616 088.31767256415 +41.46125378257 14.8129 14.2124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198308_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198308_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:42:31.59 +41:47:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.572 192857917222804096 085.63183763419 +41.79599060573 14.3975 13.5331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198310_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198313_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198313_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:40:49.16 +47:49:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.947 210661931053356160 085.20514297955 +47.82278315724 14.7839 13.9704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198317_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198317_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:25:13.69 +43:32:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.185 207733038237275392 081.30709454827 +43.54636738326 14.3684 13.4256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198323_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198323_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198328_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198328_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:18:54.48 +46:34:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.398 211895686181692288 079.72691377801 +46.58144134738 14.6253 13.7195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198337_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:09.32 +47:01:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.154 209676665556055552 086.78937106254 +47.02441587096 14.6563 13.7357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198353_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198353_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:47:42.65 +45:18:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.703 197242322916702848 086.92761567750 +45.30695470646 14.8023 13.8496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198362_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:04.22 +47:55:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.898 212543573407064960 081.01793814414 +47.93204809336 14.4423 13.5663 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#
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Considering the candidate 198364_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198364_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 198401_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 198401_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:24:23.68 +45:37:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.039 208931707774085888 081.09866894251 +45.62895522594 14.6621 14.0609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198404_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 198404_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:14:59.11 +46:47:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:37:56.95 +44:41:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:57:24.00 +48:22:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
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Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:27:04.79 +50:07:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:21:29.93 +43:44:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 05:59:44.11 +47:37:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-15_22-38-57_20.00sec_-4.90C_LIGHTs_0073 did not pass the final checks
**** FOUND 06:26:01.82 +50:29:26.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 15s
make_report_in_HTML.sh TOTAL: 455s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:31:36.99 +49:45:23.2
05:44:32.52 +42:54:21.0
05:30:20.12 +47:39:01.4
05:51:28.09 +45:11:26.9
06:17:46.27 +40:58:41.6
06:14:06.03 +47:38:25.0
05:53:43.51 +47:05:38.4
05:44:06.49 +47:04:04.1
06:13:25.89 +44:01:20.8
05:50:20.66 +46:40:54.2
05:47:36.70 +49:32:39.0
05:47:24.41 +48:07:02.8
06:06:24.50 +44:04:01.5
06:18:41.62 +42:18:28.3
06:12:57.22 +46:18:37.3
06:12:04.54 +50:30:16.5
05:30:39.45 +45:52:04.6
05:51:33.26 +43:10:28.5
06:31:45.58 +48:30:01.6
06:17:25.77 +46:39:38.7
05:52:55.76 +51:09:50.4
05:45:52.03 +50:23:47.7
05:38:30.98 +48:42:02.0
06:04:53.14 +50:08:48.5
05:33:14.93 +46:13:28.7
05:28:04.14 +49:28:30.3
05:32:56.99 +44:10:54.0
06:07:02.46 +48:02:59.7
05:18:32.90 +46:17:01.2
05:27:16.23 +45:33:34.8
06:09:22.20 +49:25:25.9
05:51:38.20 +48:20:09.6
05:57:08.99 +46:13:43.9
05:37:23.00 +46:49:18.6
05:25:37.74 +45:40:57.1
06:36:59.28 +48:07:03.5
06:02:11.16 +46:42:58.7
06:02:54.44 +43:29:35.8
05:49:29.04 +44:16:20.0
05:40:02.86 +50:02:05.2
05:40:51.33 +48:19:22.5
05:42:07.68 +50:04:32.6
05:51:18.38 +46:14:41.3
05:48:45.97 +46:35:01.8
05:28:43.89 +41:18:09.8
05:43:47.24 +43:32:42.2
05:48:04.14 +43:19:50.8
05:57:40.04 +50:14:52.0
05:28:01.35 +48:14:59.2
06:26:19.91 +41:59:10.9
05:53:06.77 +44:56:01.4
05:28:47.96 +44:55:15.4
06:01:32.43 +47:32:27.1
05:27:50.96 +42:20:27.0
05:27:26.09 +44:48:53.3
05:28:11.76 +43:27:56.0
05:55:42.92 +49:18:02.9
05:35:29.71 +45:58:10.6
05:39:41.69 +50:57:36.4
05:20:50.88 +44:04:37.9
05:37:28.22 +42:00:46.8
05:37:16.43 +44:02:47.0
05:28:41.39 +48:14:36.4
05:48:23.27 +49:46:57.8
05:32:56.27 +48:45:35.8
06:02:32.13 +48:11:24.8
05:17:29.49 +46:59:10.6
05:50:28.75 +44:11:35.1
05:19:09.88 +44:39:54.1
05:23:51.96 +48:16:07.2
05:48:08.86 +44:44:55.9
05:35:36.08 +47:32:41.8
05:37:52.52 +43:02:34.8
05:34:15.74 +44:17:07.0
05:49:38.69 +47:49:50.0
05:49:06.58 +47:17:59.9
05:29:24.44 +47:58:50.5
06:08:55.89 +40:54:29.6
05:28:27.63 +43:54:02.4
05:34:19.01 +44:27:43.8
05:39:24.95 +42:39:21.0
05:36:40.86 +50:02:55.2
06:04:15.56 +46:54:37.4
05:58:09.63 +48:37:13.4
05:33:11.73 +45:37:47.9
05:27:14.98 +48:02:46.2
06:10:43.27 +49:06:27.8
06:00:25.51 +50:29:57.9
05:28:03.28 +44:53:45.7
05:54:47.49 +47:47:13.1
05:30:04.70 +47:45:35.3
05:22:57.33 +48:35:36.8
06:10:45.09 +48:16:56.9
05:20:41.35 +48:03:51.5
05:39:31.99 +44:38:43.1
05:51:25.10 +42:52:21.2
05:54:26.96 +44:46:43.1
05:58:08.79 +48:58:10.6
06:21:46.53 +48:41:42.7
05:47:16.19 +45:37:45.1
06:07:54.33 +45:58:50.4
06:09:37.27 +50:22:55.0
05:43:59.64 +44:30:08.4
05:37:41.19 +45:58:10.3
05:37:35.34 +49:26:16.5
06:37:22.56 +44:41:37.7
05:18:46.69 +43:17:58.3
06:05:19.94 +49:43:46.5
05:57:36.56 +48:48:22.5
05:53:04.37 +46:18:46.6
05:47:45.85 +45:04:50.4
06:16:35.99 +46:36:14.4
05:59:33.99 +48:16:27.8
05:32:36.54 +42:49:48.1
06:05:14.69 +48:16:58.6
05:54:17.81 +49:03:41.5
05:40:08.71 +43:50:37.5
05:59:14.58 +47:08:48.4
06:40:23.63 +49:50:43.3
05:20:05.30 +42:17:47.6
05:33:27.87 +48:41:06.4
05:23:45.81 +43:17:54.7
05:28:02.88 +42:26:37.1
05:43:50.68 +50:03:10.9
05:32:08.85 +41:32:46.2
05:46:07.26 +48:57:19.0
06:10:07.33 +44:01:21.5
05:38:28.10 +45:02:32.3
06:00:00.48 +42:03:22.6
06:48:54.16 +49:20:22.7
05:59:03.62 +45:50:39.5
05:28:34.83 +48:03:31.2
05:34:13.08 +50:14:25.3
05:40:14.62 +41:32:17.8
06:21:42.80 +40:56:53.7
05:38:19.58 +42:29:14.4
06:28:34.71 +47:18:32.1
05:37:17.60 +44:28:42.7
06:15:04.64 +44:49:06.3
06:03:33.70 +45:26:33.6
05:36:14.61 +42:43:35.7
05:32:28.83 +47:51:04.9
05:23:12.18 +48:12:27.1
06:03:39.40 +45:55:22.7
05:59:32.05 +48:16:11.1
06:43:51.18 +48:22:27.1
06:34:52.65 +41:24:32.0
05:34:45.14 +46:34:29.4
05:17:09.47 +45:22:34.8
06:14:47.66 +44:30:39.3
05:35:09.24 +46:30:58.5
06:24:43.89 +43:30:23.1
05:26:46.59 +48:28:08.7
05:37:30.42 +44:27:04.5
05:44:16.20 +51:00:43.0
06:35:53.18 +43:17:38.7
06:03:26.78 +47:27:54.0
06:03:07.20 +41:11:11.9
05:54:28.13 +43:33:42.0
05:53:51.68 +48:45:15.7
06:11:46.84 +45:23:10.4
05:18:45.62 +47:29:04.3
05:53:36.56 +42:34:46.6
05:51:09.60 +48:36:28.0
05:56:51.15 +47:43:17.7
05:30:43.09 +51:06:58.1
06:34:07.99 +45:28:14.4
06:07:24.15 +50:24:29.1
05:23:56.27 +49:22:51.6
05:30:13.04 +49:03:30.7
05:36:49.29 +41:40:01.2
05:53:51.16 +47:35:30.4
05:38:26.14 +42:41:34.2
06:04:31.95 +46:49:07.7
05:22:27.28 +46:19:53.7
05:22:34.77 +48:10:09.5
05:24:24.88 +44:33:55.1
05:32:49.84 +45:19:42.5
05:55:17.89 +42:29:28.8
05:51:42.81 +41:57:24.6
06:09:51.89 +46:34:26.9
########### Completed Aur-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:31:36.99 +49:45:23.2
05:44:32.52 +42:54:21.0
05:30:20.12 +47:39:01.4
05:51:28.09 +45:11:26.9
06:17:46.27 +40:58:41.6
06:14:06.03 +47:38:25.0
05:53:43.51 +47:05:38.4
05:44:06.49 +47:04:04.1
06:13:25.89 +44:01:20.8
05:50:20.66 +46:40:54.2
05:47:36.70 +49:32:39.0
05:47:24.41 +48:07:02.8
06:06:24.50 +44:04:01.5
06:18:41.62 +42:18:28.3
06:12:57.22 +46:18:37.3
06:12:04.54 +50:30:16.5
05:30:39.45 +45:52:04.6
05:51:33.26 +43:10:28.5
06:31:45.58 +48:30:01.6
06:17:25.77 +46:39:38.7
05:52:55.76 +51:09:50.4
05:45:52.03 +50:23:47.7
05:38:30.98 +48:42:02.0
06:04:53.14 +50:08:48.5
05:33:14.93 +46:13:28.7
05:28:04.14 +49:28:30.3
05:32:56.99 +44:10:54.0
06:07:02.46 +48:02:59.7
05:18:32.90 +46:17:01.2
05:27:16.23 +45:33:34.8
06:09:22.20 +49:25:25.9
05:51:38.20 +48:20:09.6
05:57:08.99 +46:13:43.9
05:37:23.00 +46:49:18.6
05:25:37.74 +45:40:57.1
06:36:59.28 +48:07:03.5
06:02:11.16 +46:42:58.7
06:02:54.44 +43:29:35.8
05:49:29.04 +44:16:20.0
05:40:02.86 +50:02:05.2
05:40:51.33 +48:19:22.5
05:42:07.68 +50:04:32.6
05:51:18.38 +46:14:41.3
05:48:45.97 +46:35:01.8
05:28:43.89 +41:18:09.8
05:43:47.24 +43:32:42.2
05:48:04.14 +43:19:50.8
05:57:40.04 +50:14:52.0
05:28:01.35 +48:14:59.2
06:26:19.91 +41:59:10.9
05:53:06.77 +44:56:01.4
05:28:47.96 +44:55:15.4
06:01:32.43 +47:32:27.1
05:27:50.96 +42:20:27.0
05:27:26.09 +44:48:53.3
05:28:11.76 +43:27:56.0
05:55:42.92 +49:18:02.9
05:35:29.71 +45:58:10.6
05:39:41.69 +50:57:36.4
05:20:50.88 +44:04:37.9
05:37:28.22 +42:00:46.8
05:37:16.43 +44:02:47.0
05:28:41.39 +48:14:36.4
05:48:23.27 +49:46:57.8
05:32:56.27 +48:45:35.8
06:02:32.13 +48:11:24.8
05:17:29.49 +46:59:10.6
05:50:28.75 +44:11:35.1
05:19:09.88 +44:39:54.1
05:23:51.96 +48:16:07.2
05:48:08.86 +44:44:55.9
05:35:36.08 +47:32:41.8
05:37:52.52 +43:02:34.8
05:34:15.74 +44:17:07.0
05:49:38.69 +47:49:50.0
05:49:06.58 +47:17:59.9
05:29:24.44 +47:58:50.5
06:08:55.89 +40:54:29.6
05:28:27.63 +43:54:02.4
05:34:19.01 +44:27:43.8
05:39:24.95 +42:39:21.0
05:36:40.86 +50:02:55.2
06:04:15.56 +46:54:37.4
05:58:09.63 +48:37:13.4
05:33:11.73 +45:37:47.9
05:27:14.98 +48:02:46.2
06:10:43.27 +49:06:27.8
06:00:25.51 +50:29:57.9
05:28:03.28 +44:53:45.7
05:54:47.49 +47:47:13.1
05:30:04.70 +47:45:35.3
05:22:57.33 +48:35:36.8
06:10:45.09 +48:16:56.9
05:20:41.35 +48:03:51.5
05:39:31.99 +44:38:43.1
05:51:25.10 +42:52:21.2
05:54:26.96 +44:46:43.1
05:58:08.79 +48:58:10.6
06:21:46.53 +48:41:42.7
05:47:16.19 +45:37:45.1
06:07:54.33 +45:58:50.4
06:09:37.27 +50:22:55.0
05:43:59.64 +44:30:08.4
05:37:41.19 +45:58:10.3
05:37:35.34 +49:26:16.5
06:37:22.56 +44:41:37.7
05:18:46.69 +43:17:58.3
06:05:19.94 +49:43:46.5
05:57:36.56 +48:48:22.5
05:53:04.37 +46:18:46.6
05:47:45.85 +45:04:50.4
06:16:35.99 +46:36:14.4
05:59:33.99 +48:16:27.8
05:32:36.54 +42:49:48.1
06:05:14.69 +48:16:58.6
05:54:17.81 +49:03:41.5
05:40:08.71 +43:50:37.5
05:59:14.58 +47:08:48.4
06:40:23.63 +49:50:43.3
05:20:05.30 +42:17:47.6
05:33:27.87 +48:41:06.4
05:23:45.81 +43:17:54.7
05:28:02.88 +42:26:37.1
05:43:50.68 +50:03:10.9
05:32:08.85 +41:32:46.2
05:46:07.26 +48:57:19.0
06:10:07.33 +44:01:21.5
05:38:28.10 +45:02:32.3
06:00:00.48 +42:03:22.6
06:48:54.16 +49:20:22.7
05:59:03.62 +45:50:39.5
05:28:34.83 +48:03:31.2
05:34:13.08 +50:14:25.3
05:40:14.62 +41:32:17.8
06:21:42.80 +40:56:53.7
05:38:19.58 +42:29:14.4
06:28:34.71 +47:18:32.1
05:37:17.60 +44:28:42.7
06:15:04.64 +44:49:06.3
06:03:33.70 +45:26:33.6
05:36:14.61 +42:43:35.7
05:32:28.83 +47:51:04.9
05:23:12.18 +48:12:27.1
06:03:39.40 +45:55:22.7
05:59:32.05 +48:16:11.1
06:43:51.18 +48:22:27.1
06:34:52.65 +41:24:32.0
05:34:45.14 +46:34:29.4
05:17:09.47 +45:22:34.8
06:14:47.66 +44:30:39.3
05:35:09.24 +46:30:58.5
06:24:43.89 +43:30:23.1
05:26:46.59 +48:28:08.7
05:37:30.42 +44:27:04.5
05:44:16.20 +51:00:43.0
06:35:53.18 +43:17:38.7
06:03:26.78 +47:27:54.0
06:03:07.20 +41:11:11.9
05:54:28.13 +43:33:42.0
05:53:51.68 +48:45:15.7
06:11:46.84 +45:23:10.4
05:18:45.62 +47:29:04.3
05:53:36.56 +42:34:46.6
05:51:09.60 +48:36:28.0
05:56:51.15 +47:43:17.7
05:30:43.09 +51:06:58.1
06:34:07.99 +45:28:14.4
06:07:24.15 +50:24:29.1
05:23:56.27 +49:22:51.6
05:30:13.04 +49:03:30.7
05:36:49.29 +41:40:01.2
05:53:51.16 +47:35:30.4
05:38:26.14 +42:41:34.2
06:04:31.95 +46:49:07.7
05:22:27.28 +46:19:53.7
05:22:34.77 +48:10:09.5
05:24:24.88 +44:33:55.1
05:32:49.84 +45:19:42.5
05:55:17.89 +42:29:28.8
05:51:42.81 +41:57:24.6
06:09:51.89 +46:34:26.9
###################################################################################
05:31:36.99 +49:45:23.2 -- not an asteroid (will add it to exclusion list)
05:44:32.52 +42:54:21.0 -- not an asteroid (will add it to exclusion list)
05:30:20.12 +47:39:01.4 -- not an asteroid (will add it to exclusion list)
05:51:28.09 +45:11:26.9 -- not an asteroid (will add it to exclusion list)
06:17:46.27 +40:58:41.6 -- not an asteroid (will add it to exclusion list)
06:14:06.03 +47:38:25.0 -- not an asteroid (will add it to exclusion list)
05:53:43.51 +47:05:38.4 -- not an asteroid (will add it to exclusion list)
05:44:06.49 +47:04:04.1 -- not an asteroid (will add it to exclusion list)
06:13:25.89 +44:01:20.8 -- not an asteroid (will add it to exclusion list)
05:50:20.66 +46:40:54.2 -- not an asteroid (will add it to exclusion list)
05:47:36.70 +49:32:39.0 -- not an asteroid (will add it to exclusion list)
05:47:24.41 +48:07:02.8 -- not an asteroid (will add it to exclusion list)
06:06:24.50 +44:04:01.5 -- not an asteroid (will add it to exclusion list)
06:18:41.62 +42:18:28.3 -- not an asteroid (will add it to exclusion list)
06:12:57.22 +46:18:37.3 -- not an asteroid (will add it to exclusion list)
06:12:04.54 +50:30:16.5 -- not an asteroid (will add it to exclusion list)
05:30:39.45 +45:52:04.6 -- not an asteroid (will add it to exclusion list)
05:51:33.26 +43:10:28.5 -- not an asteroid (will add it to exclusion list)
06:31:45.58 +48:30:01.6 -- not an asteroid (will add it to exclusion list)
06:17:25.77 +46:39:38.7 -- not an asteroid (will add it to exclusion list)
05:52:55.76 +51:09:50.4 -- not an asteroid (will add it to exclusion list)
05:45:52.03 +50:23:47.7 -- not an asteroid (will add it to exclusion list)
05:38:30.98 +48:42:02.0 -- not an asteroid (will add it to exclusion list)
06:04:53.14 +50:08:48.5 -- not an asteroid (will add it to exclusion list)
05:33:14.93 +46:13:28.7 -- not an asteroid (will add it to exclusion list)
05:28:04.14 +49:28:30.3 -- not an asteroid (will add it to exclusion list)
05:32:56.99 +44:10:54.0 -- not an asteroid (will add it to exclusion list)
06:07:02.46 +48:02:59.7 -- not an asteroid (will add it to exclusion list)
05:18:32.90 +46:17:01.2 -- not an asteroid (will add it to exclusion list)
05:27:16.23 +45:33:34.8 -- not an asteroid (will add it to exclusion list)
06:09:22.20 +49:25:25.9 -- not an asteroid (will add it to exclusion list)
05:51:38.20 +48:20:09.6 -- not an asteroid (will add it to exclusion list)
05:57:08.99 +46:13:43.9 -- not an asteroid (will add it to exclusion list)
05:37:23.00 +46:49:18.6 -- not an asteroid (will add it to exclusion list)
05:25:37.74 +45:40:57.1 -- not an asteroid (will add it to exclusion list)
06:36:59.28 +48:07:03.5 -- not an asteroid (will add it to exclusion list)
06:02:11.16 +46:42:58.7 -- not an asteroid (will add it to exclusion list)
06:02:54.44 +43:29:35.8 -- not an asteroid (will add it to exclusion list)
05:49:29.04 +44:16:20.0 -- not an asteroid (will add it to exclusion list)
05:40:02.86 +50:02:05.2 -- not an asteroid (will add it to exclusion list)
05:40:51.33 +48:19:22.5 -- not an asteroid (will add it to exclusion list)
05:42:07.68 +50:04:32.6 -- not an asteroid (will add it to exclusion list)
05:51:18.38 +46:14:41.3 -- not an asteroid (will add it to exclusion list)
05:48:45.97 +46:35:01.8 -- not an asteroid (will add it to exclusion list)
05:28:43.89 +41:18:09.8 -- not an asteroid (will add it to exclusion list)
05:43:47.24 +43:32:42.2 -- not an asteroid (will add it to exclusion list)
05:48:04.14 +43:19:50.8 -- not an asteroid (will add it to exclusion list)
05:57:40.04 +50:14:52.0 -- not an asteroid (will add it to exclusion list)
05:28:01.35 +48:14:59.2 -- not an asteroid (will add it to exclusion list)
06:26:19.91 +41:59:10.9 -- not an asteroid (will add it to exclusion list)
05:53:06.77 +44:56:01.4 -- not an asteroid (will add it to exclusion list)
05:28:47.96 +44:55:15.4 -- not an asteroid (will add it to exclusion list)
06:01:32.43 +47:32:27.1 -- not an asteroid (will add it to exclusion list)
05:27:50.96 +42:20:27.0 -- not an asteroid (will add it to exclusion list)
05:27:26.09 +44:48:53.3 -- not an asteroid (will add it to exclusion list)
05:28:11.76 +43:27:56.0 -- not an asteroid (will add it to exclusion list)
05:55:42.92 +49:18:02.9 -- not an asteroid (will add it to exclusion list)
05:35:29.71 +45:58:10.6 -- not an asteroid (will add it to exclusion list)
05:39:41.69 +50:57:36.4 -- not an asteroid (will add it to exclusion list)
05:20:50.88 +44:04:37.9 -- not an asteroid (will add it to exclusion list)
05:37:28.22 +42:00:46.8 -- not an asteroid (will add it to exclusion list)
05:37:16.43 +44:02:47.0 -- not an asteroid (will add it to exclusion list)
05:28:41.39 +48:14:36.4 -- not an asteroid (will add it to exclusion list)
05:48:23.27 +49:46:57.8 -- not an asteroid (will add it to exclusion list)
05:32:56.27 +48:45:35.8 -- not an asteroid (will add it to exclusion list)
06:02:32.13 +48:11:24.8 -- not an asteroid (will add it to exclusion list)
05:17:29.49 +46:59:10.6 -- not an asteroid (will add it to exclusion list)
05:50:28.75 +44:11:35.1 -- not an asteroid (will add it to exclusion list)
05:19:09.88 +44:39:54.1 -- not an asteroid (will add it to exclusion list)
05:23:51.96 +48:16:07.2 -- not an asteroid (will add it to exclusion list)
05:48:08.86 +44:44:55.9 -- not an asteroid (will add it to exclusion list)
05:35:36.08 +47:32:41.8 -- not an asteroid (will add it to exclusion list)
05:37:52.52 +43:02:34.8 -- not an asteroid (will add it to exclusion list)
05:34:15.74 +44:17:07.0 -- not an asteroid (will add it to exclusion list)
05:49:38.69 +47:49:50.0 -- not an asteroid (will add it to exclusion list)
05:49:06.58 +47:17:59.9 -- not an asteroid (will add it to exclusion list)
05:29:24.44 +47:58:50.5 -- not an asteroid (will add it to exclusion list)
06:08:55.89 +40:54:29.6 -- not an asteroid (will add it to exclusion list)
05:28:27.63 +43:54:02.4 -- not an asteroid (will add it to exclusion list)
05:34:19.01 +44:27:43.8 -- not an asteroid (will add it to exclusion list)
05:39:24.95 +42:39:21.0 -- not an asteroid (will add it to exclusion list)
05:36:40.86 +50:02:55.2 -- not an asteroid (will add it to exclusion list)
06:04:15.56 +46:54:37.4 -- not an asteroid (will add it to exclusion list)
05:58:09.63 +48:37:13.4 -- not an asteroid (will add it to exclusion list)
05:33:11.73 +45:37:47.9 -- not an asteroid (will add it to exclusion list)
05:27:14.98 +48:02:46.2 -- not an asteroid (will add it to exclusion list)
06:10:43.27 +49:06:27.8 -- not an asteroid (will add it to exclusion list)
06:00:25.51 +50:29:57.9 -- not an asteroid (will add it to exclusion list)
05:28:03.28 +44:53:45.7 -- not an asteroid (will add it to exclusion list)
05:54:47.49 +47:47:13.1 -- not an asteroid (will add it to exclusion list)
05:30:04.70 +47:45:35.3 -- not an asteroid (will add it to exclusion list)
05:22:57.33 +48:35:36.8 -- not an asteroid (will add it to exclusion list)
06:10:45.09 +48:16:56.9 -- not an asteroid (will add it to exclusion list)
05:20:41.35 +48:03:51.5 -- not an asteroid (will add it to exclusion list)
05:39:31.99 +44:38:43.1 -- not an asteroid (will add it to exclusion list)
05:51:25.10 +42:52:21.2 -- not an asteroid (will add it to exclusion list)
05:54:26.96 +44:46:43.1 -- not an asteroid (will add it to exclusion list)
05:58:08.79 +48:58:10.6 -- not an asteroid (will add it to exclusion list)
06:21:46.53 +48:41:42.7 -- not an asteroid (will add it to exclusion list)
05:47:16.19 +45:37:45.1 -- not an asteroid (will add it to exclusion list)
06:07:54.33 +45:58:50.4 -- not an asteroid (will add it to exclusion list)
06:09:37.27 +50:22:55.0 -- not an asteroid (will add it to exclusion list)
05:43:59.64 +44:30:08.4 -- not an asteroid (will add it to exclusion list)
05:37:41.19 +45:58:10.3 -- not an asteroid (will add it to exclusion list)
05:37:35.34 +49:26:16.5 -- not an asteroid (will add it to exclusion list)
06:37:22.56 +44:41:37.7 -- not an asteroid (will add it to exclusion list)
05:18:46.69 +43:17:58.3 -- not an asteroid (will add it to exclusion list)
06:05:19.94 +49:43:46.5 -- not an asteroid (will add it to exclusion list)
05:57:36.56 +48:48:22.5 -- not an asteroid (will add it to exclusion list)
05:53:04.37 +46:18:46.6 -- not an asteroid (will add it to exclusion list)
05:47:45.85 +45:04:50.4 -- not an asteroid (will add it to exclusion list)
06:16:35.99 +46:36:14.4 -- not an asteroid (will add it to exclusion list)
05:59:33.99 +48:16:27.8 -- not an asteroid (will add it to exclusion list)
05:32:36.54 +42:49:48.1 -- not an asteroid (will add it to exclusion list)
06:05:14.69 +48:16:58.6 -- not an asteroid (will add it to exclusion list)
05:54:17.81 +49:03:41.5 -- not an asteroid (will add it to exclusion list)
05:40:08.71 +43:50:37.5 -- not an asteroid (will add it to exclusion list)
05:59:14.58 +47:08:48.4 -- not an asteroid (will add it to exclusion list)
06:40:23.63 +49:50:43.3 -- not an asteroid (will add it to exclusion list)
05:20:05.30 +42:17:47.6 -- not an asteroid (will add it to exclusion list)
05:33:27.87 +48:41:06.4 -- not an asteroid (will add it to exclusion list)
05:23:45.81 +43:17:54.7 -- not an asteroid (will add it to exclusion list)
05:28:02.88 +42:26:37.1 -- not an asteroid (will add it to exclusion list)
05:43:50.68 +50:03:10.9 -- not an asteroid (will add it to exclusion list)
05:32:08.85 +41:32:46.2 -- not an asteroid (will add it to exclusion list)
05:46:07.26 +48:57:19.0 -- not an asteroid (will add it to exclusion list)
06:10:07.33 +44:01:21.5 -- not an asteroid (will add it to exclusion list)
05:38:28.10 +45:02:32.3 -- not an asteroid (will add it to exclusion list)
06:00:00.48 +42:03:22.6 -- not an asteroid (will add it to exclusion list)
06:48:54.16 +49:20:22.7 -- not an asteroid (will add it to exclusion list)
05:59:03.62 +45:50:39.5 -- not an asteroid (will add it to exclusion list)
05:28:34.83 +48:03:31.2 -- not an asteroid (will add it to exclusion list)
05:34:13.08 +50:14:25.3 -- not an asteroid (will add it to exclusion list)
05:40:14.62 +41:32:17.8 -- not an asteroid (will add it to exclusion list)
06:21:42.80 +40:56:53.7 -- not an asteroid (will add it to exclusion list)
05:38:19.58 +42:29:14.4 -- not an asteroid (will add it to exclusion list)
06:28:34.71 +47:18:32.1 -- not an asteroid (will add it to exclusion list)
05:37:17.60 +44:28:42.7 -- not an asteroid (will add it to exclusion list)
06:15:04.64 +44:49:06.3 -- not an asteroid (will add it to exclusion list)
06:03:33.70 +45:26:33.6 -- not an asteroid (will add it to exclusion list)
05:36:14.61 +42:43:35.7 -- not an asteroid (will add it to exclusion list)
05:32:28.83 +47:51:04.9 -- not an asteroid (will add it to exclusion list)
05:23:12.18 +48:12:27.1 -- not an asteroid (will add it to exclusion list)
06:03:39.40 +45:55:22.7 -- not an asteroid (will add it to exclusion list)
05:59:32.05 +48:16:11.1 -- not an asteroid (will add it to exclusion list)
06:43:51.18 +48:22:27.1 -- not an asteroid (will add it to exclusion list)
06:34:52.65 +41:24:32.0 -- not an asteroid (will add it to exclusion list)
05:34:45.14 +46:34:29.4 -- not an asteroid (will add it to exclusion list)
05:17:09.47 +45:22:34.8 -- not an asteroid (will add it to exclusion list)
06:14:47.66 +44:30:39.3 -- not an asteroid (will add it to exclusion list)
05:35:09.24 +46:30:58.5 -- not an asteroid (will add it to exclusion list)
06:24:43.89 +43:30:23.1 -- not an asteroid (will add it to exclusion list)
05:26:46.59 +48:28:08.7 -- not an asteroid (will add it to exclusion list)
05:37:30.42 +44:27:04.5 -- not an asteroid (will add it to exclusion list)
05:44:16.20 +51:00:43.0 -- not an asteroid (will add it to exclusion list)
06:35:53.18 +43:17:38.7 -- not an asteroid (will add it to exclusion list)
06:03:26.78 +47:27:54.0 -- not an asteroid (will add it to exclusion list)
06:03:07.20 +41:11:11.9 -- not an asteroid (will add it to exclusion list)
05:54:28.13 +43:33:42.0 -- not an asteroid (will add it to exclusion list)
05:53:51.68 +48:45:15.7 -- not an asteroid (will add it to exclusion list)
06:11:46.84 +45:23:10.4 -- not an asteroid (will add it to exclusion list)
05:18:45.62 +47:29:04.3 -- not an asteroid (will add it to exclusion list)
05:53:36.56 +42:34:46.6 -- not an asteroid (will add it to exclusion list)
05:51:09.60 +48:36:28.0 -- not an asteroid (will add it to exclusion list)
05:56:51.15 +47:43:17.7 -- not an asteroid (will add it to exclusion list)
05:30:43.09 +51:06:58.1 -- not an asteroid (will add it to exclusion list)
06:34:07.99 +45:28:14.4 -- not an asteroid (will add it to exclusion list)
06:07:24.15 +50:24:29.1 -- not an asteroid (will add it to exclusion list)
05:23:56.27 +49:22:51.6 -- not an asteroid (will add it to exclusion list)
05:30:13.04 +49:03:30.7 -- not an asteroid (will add it to exclusion list)
05:36:49.29 +41:40:01.2 -- not an asteroid (will add it to exclusion list)
05:53:51.16 +47:35:30.4 -- not an asteroid (will add it to exclusion list)
05:38:26.14 +42:41:34.2 -- not an asteroid (will add it to exclusion list)
06:04:31.95 +46:49:07.7 -- not an asteroid (will add it to exclusion list)
05:22:27.28 +46:19:53.7 -- not an asteroid (will add it to exclusion list)
05:22:34.77 +48:10:09.5 -- not an asteroid (will add it to exclusion list)
05:24:24.88 +44:33:55.1 -- not an asteroid (will add it to exclusion list)
05:32:49.84 +45:19:42.5 -- not an asteroid (will add it to exclusion list)
05:55:17.89 +42:29:28.8 -- not an asteroid (will add it to exclusion list)
05:51:42.81 +41:57:24.6 -- not an asteroid (will add it to exclusion list)
06:09:51.89 +46:34:26.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:17:09.47 +45:22:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.49 +46:59:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:32.90 +46:17:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:45.62 +47:29:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:46.69 +43:17:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.88 +44:39:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:05.30 +42:17:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:41.35 +48:03:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.88 +44:04:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:27.28 +46:19:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:34.77 +48:10:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:57.33 +48:35:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:12.18 +48:12:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:45.81 +43:17:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:51.96 +48:16:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:56.27 +49:22:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:24.88 +44:33:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.74 +45:40:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:46.59 +48:28:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:14.98 +48:02:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:16.23 +45:33:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.09 +44:48:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:50.96 +42:20:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.35 +48:14:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:02.88 +42:26:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:03.28 +44:53:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.14 +49:28:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.76 +43:27:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:27.63 +43:54:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:34.83 +48:03:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:41.39 +48:14:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:43.89 +41:18:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:47.96 +44:55:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:24.44 +47:58:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:04.70 +47:45:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:13.04 +49:03:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:20.12 +47:39:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:39.45 +45:52:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:43.09 +51:06:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:36.99 +49:45:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:08.85 +41:32:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:28.83 +47:51:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:36.54 +42:49:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:49.84 +45:19:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.27 +48:45:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.99 +44:10:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:11.73 +45:37:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:14.93 +46:13:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:27.87 +48:41:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:13.08 +50:14:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.74 +44:17:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.01 +44:27:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:45.14 +46:34:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:09.24 +46:30:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:29.71 +45:58:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:36.08 +47:32:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:14.61 +42:43:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.86 +50:02:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:49.29 +41:40:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.43 +44:02:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:17.60 +44:28:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:23.00 +46:49:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:28.22 +42:00:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:30.42 +44:27:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:35.34 +49:26:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.19 +45:58:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.52 +43:02:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:19.58 +42:29:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:26.14 +42:41:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:28.10 +45:02:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:30.98 +48:42:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:24.95 +42:39:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:31.99 +44:38:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:41.69 +50:57:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.86 +50:02:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:08.71 +43:50:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:14.62 +41:32:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:51.33 +48:19:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:07.68 +50:04:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.24 +43:32:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:50.68 +50:03:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:59.64 +44:30:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:06.49 +47:04:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:16.20 +51:00:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:32.52 +42:54:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:52.03 +50:23:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:07.26 +48:57:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:16.19 +45:37:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:24.41 +48:07:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:36.70 +49:32:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:45.85 +45:04:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.14 +43:19:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:08.86 +44:44:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.27 +49:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:45.97 +46:35:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.58 +47:17:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:29.04 +44:16:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.69 +47:49:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:20.66 +46:40:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.75 +44:11:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:09.60 +48:36:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.38 +46:14:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:25.10 +42:52:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:28.09 +45:11:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:33.26 +43:10:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:38.20 +48:20:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:42.81 +41:57:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:55.76 +51:09:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.37 +46:18:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.77 +44:56:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:36.56 +42:34:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:43.51 +47:05:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:51.16 +47:35:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:51.68 +48:45:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:17.81 +49:03:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:26.96 +44:46:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:28.13 +43:33:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:47.49 +47:47:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:17.89 +42:29:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:42.92 +49:18:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:51.15 +47:43:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:08.99 +46:13:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:36.56 +48:48:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:40.04 +50:14:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:08.79 +48:58:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.63 +48:37:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:03.62 +45:50:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:14.58 +47:08:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:32.05 +48:16:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:33.99 +48:16:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:00.48 +42:03:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:25.51 +50:29:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.43 +47:32:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:11.16 +46:42:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.13 +48:11:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:54.44 +43:29:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:07.20 +41:11:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:26.78 +47:27:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:33.70 +45:26:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:39.40 +45:55:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.56 +46:54:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:31.95 +46:49:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:53.14 +50:08:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:14.69 +48:16:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:19.94 +49:43:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:24.50 +44:04:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:02.46 +48:02:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:24.15 +50:24:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.33 +45:58:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:55.89 +40:54:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:22.20 +49:25:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:37.27 +50:22:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.89 +46:34:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:07.33 +44:01:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:43.27 +49:06:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.09 +48:16:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:46.84 +45:23:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:04.54 +50:30:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:57.22 +46:18:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:25.89 +44:01:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:06.03 +47:38:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:47.66 +44:30:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:04.64 +44:49:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:35.99 +46:36:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:25.77 +46:39:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:46.27 +40:58:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:41.62 +42:18:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:42.80 +40:56:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:46.53 +48:41:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:43.89 +43:30:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.91 +41:59:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:34.71 +47:18:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:45.58 +48:30:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:07.99 +45:28:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:52.65 +41:24:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:53.18 +43:17:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:59.28 +48:07:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:22.56 +44:41:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:23.63 +49:50:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:51.18 +48:22:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:54.16 +49:20:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:17:09.47 +45:22:34.8 -- not a known variable star
05:17:29.49 +46:59:10.6 -- not a known variable star
05:18:32.90 +46:17:01.2 -- not a known variable star
05:18:45.62 +47:29:04.3 -- not a known variable star
05:18:46.69 +43:17:58.3 -- not a known variable star
05:19:09.88 +44:39:54.1 -- not a known variable star
05:20:05.30 +42:17:47.6 -- not a known variable star
05:20:41.35 +48:03:51.5 -- not a known variable star
05:20:50.88 +44:04:37.9 -- not a known variable star
05:22:27.28 +46:19:53.7 -- not a known variable star
05:22:34.77 +48:10:09.5 -- not a known variable star
05:22:57.33 +48:35:36.8 -- not a known variable star
05:23:12.18 +48:12:27.1 -- not a known variable star
05:23:45.81 +43:17:54.7 -- not a known variable star
05:23:51.96 +48:16:07.2 -- not a known variable star
05:23:56.27 +49:22:51.6 -- not a known variable star
05:24:24.88 +44:33:55.1 -- a known variable star
05:25:37.74 +45:40:57.1 -- not a known variable star
05:26:46.59 +48:28:08.7 -- not a known variable star
05:27:14.98 +48:02:46.2 -- not a known variable star
05:27:16.23 +45:33:34.8 -- not a known variable star
05:27:26.09 +44:48:53.3 -- not a known variable star
05:27:50.96 +42:20:27.0 -- not a known variable star
05:28:01.35 +48:14:59.2 -- a known variable star
05:28:02.88 +42:26:37.1 -- not a known variable star
05:28:03.28 +44:53:45.7 -- not a known variable star
05:28:04.14 +49:28:30.3 -- not a known variable star
05:28:11.76 +43:27:56.0 -- not a known variable star
05:28:27.63 +43:54:02.4 -- not a known variable star
05:28:34.83 +48:03:31.2 -- not a known variable star
05:28:41.39 +48:14:36.4 -- not a known variable star
05:28:43.89 +41:18:09.8 -- not a known variable star
05:28:47.96 +44:55:15.4 -- not a known variable star
05:29:24.44 +47:58:50.5 -- not a known variable star
05:30:04.70 +47:45:35.3 -- not a known variable star
05:30:13.04 +49:03:30.7 -- not a known variable star
05:30:20.12 +47:39:01.4 -- not a known variable star
05:30:39.45 +45:52:04.6 -- not a known variable star
05:30:43.09 +51:06:58.1 -- not a known variable star
05:31:36.99 +49:45:23.2 -- not a known variable star
05:32:08.85 +41:32:46.2 -- a known variable star
05:32:28.83 +47:51:04.9 -- not a known variable star
05:32:36.54 +42:49:48.1 -- not a known variable star
05:32:49.84 +45:19:42.5 -- not a known variable star
05:32:56.27 +48:45:35.8 -- not a known variable star
05:32:56.99 +44:10:54.0 -- not a known variable star
05:33:11.73 +45:37:47.9 -- not a known variable star
05:33:14.93 +46:13:28.7 -- a known variable star
05:33:27.87 +48:41:06.4 -- not a known variable star
05:34:13.08 +50:14:25.3 -- not a known variable star
05:34:15.74 +44:17:07.0 -- not a known variable star
05:34:19.01 +44:27:43.8 -- not a known variable star
05:34:45.14 +46:34:29.4 -- not a known variable star
05:35:09.24 +46:30:58.5 -- not a known variable star
05:35:29.71 +45:58:10.6 -- not a known variable star
05:35:36.08 +47:32:41.8 -- not a known variable star
05:36:14.61 +42:43:35.7 -- not a known variable star
05:36:40.86 +50:02:55.2 -- not a known variable star
05:36:49.29 +41:40:01.2 -- not a known variable star
05:37:16.43 +44:02:47.0 -- not a known variable star
05:37:17.60 +44:28:42.7 -- a known variable star
05:37:23.00 +46:49:18.6 -- not a known variable star
05:37:28.22 +42:00:46.8 -- not a known variable star
05:37:30.42 +44:27:04.5 -- a known variable star
05:37:35.34 +49:26:16.5 -- a known variable star
05:37:41.19 +45:58:10.3 -- not a known variable star
05:37:52.52 +43:02:34.8 -- not a known variable star
05:38:19.58 +42:29:14.4 -- not a known variable star
05:38:26.14 +42:41:34.2 -- not a known variable star
05:38:28.10 +45:02:32.3 -- not a known variable star
05:38:30.98 +48:42:02.0 -- not a known variable star
05:39:24.95 +42:39:21.0 -- not a known variable star
05:39:31.99 +44:38:43.1 -- not a known variable star
05:39:41.69 +50:57:36.4 -- not a known variable star
05:40:02.86 +50:02:05.2 -- not a known variable star
05:40:08.71 +43:50:37.5 -- not a known variable star
05:40:14.62 +41:32:17.8 -- not a known variable star
05:40:51.33 +48:19:22.5 -- not a known variable star
05:42:07.68 +50:04:32.6 -- not a known variable star
05:43:47.24 +43:32:42.2 -- not a known variable star
05:43:50.68 +50:03:10.9 -- not a known variable star
05:43:59.64 +44:30:08.4 -- a known variable star
05:44:06.49 +47:04:04.1 -- not a known variable star
05:44:16.20 +51:00:43.0 -- a known variable star
05:44:32.52 +42:54:21.0 -- not a known variable star
05:45:52.03 +50:23:47.7 -- not a known variable star
05:46:07.26 +48:57:19.0 -- not a known variable star
05:47:16.19 +45:37:45.1 -- not a known variable star
05:47:24.41 +48:07:02.8 -- not a known variable star
05:47:36.70 +49:32:39.0 -- not a known variable star
05:47:45.85 +45:04:50.4 -- not a known variable star
05:48:04.14 +43:19:50.8 -- not a known variable star
05:48:08.86 +44:44:55.9 -- not a known variable star
05:48:23.27 +49:46:57.8 -- not a known variable star
05:48:45.97 +46:35:01.8 -- a known variable star
05:49:06.58 +47:17:59.9 -- not a known variable star
05:49:29.04 +44:16:20.0 -- not a known variable star
05:49:38.69 +47:49:50.0 -- not a known variable star
05:50:20.66 +46:40:54.2 -- a known variable star
05:50:28.75 +44:11:35.1 -- a known variable star
05:51:09.60 +48:36:28.0 -- not a known variable star
05:51:18.38 +46:14:41.3 -- not a known variable star
05:51:25.10 +42:52:21.2 -- not a known variable star
05:51:28.09 +45:11:26.9 -- a known variable star
05:51:33.26 +43:10:28.5 -- not a known variable star
05:51:38.20 +48:20:09.6 -- not a known variable star
05:51:42.81 +41:57:24.6 -- not a known variable star
05:52:55.76 +51:09:50.4 -- not a known variable star
05:53:04.37 +46:18:46.6 -- not a known variable star
05:53:06.77 +44:56:01.4 -- not a known variable star
05:53:36.56 +42:34:46.6 -- a known variable star
05:53:43.51 +47:05:38.4 -- not a known variable star
05:53:51.16 +47:35:30.4 -- not a known variable star
05:53:51.68 +48:45:15.7 -- a known variable star
05:54:17.81 +49:03:41.5 -- not a known variable star
05:54:26.96 +44:46:43.1 -- not a known variable star
05:54:28.13 +43:33:42.0 -- not a known variable star
05:54:47.49 +47:47:13.1 -- not a known variable star
05:55:17.89 +42:29:28.8 -- not a known variable star
05:55:42.92 +49:18:02.9 -- not a known variable star
05:56:51.15 +47:43:17.7 -- not a known variable star
05:57:08.99 +46:13:43.9 -- not a known variable star
05:57:36.56 +48:48:22.5 -- not a known variable star
05:57:40.04 +50:14:52.0 -- a known variable star
05:58:08.79 +48:58:10.6 -- not a known variable star
05:58:09.63 +48:37:13.4 -- not a known variable star
05:59:03.62 +45:50:39.5 -- not a known variable star
05:59:14.58 +47:08:48.4 -- not a known variable star
05:59:32.05 +48:16:11.1 -- not a known variable star
05:59:33.99 +48:16:27.8 -- not a known variable star
06:00:00.48 +42:03:22.6 -- not a known variable star
06:00:25.51 +50:29:57.9 -- not a known variable star
06:01:32.43 +47:32:27.1 -- not a known variable star
06:02:11.16 +46:42:58.7 -- not a known variable star
06:02:32.13 +48:11:24.8 -- not a known variable star
06:02:54.44 +43:29:35.8 -- not a known variable star
06:03:07.20 +41:11:11.9 -- not a known variable star
06:03:26.78 +47:27:54.0 -- not a known variable star
06:03:33.70 +45:26:33.6 -- a known variable star
06:03:39.40 +45:55:22.7 -- not a known variable star
06:04:15.56 +46:54:37.4 -- not a known variable star
06:04:31.95 +46:49:07.7 -- not a known variable star
06:04:53.14 +50:08:48.5 -- not a known variable star
06:05:14.69 +48:16:58.6 -- not a known variable star
06:05:19.94 +49:43:46.5 -- not a known variable star
06:06:24.50 +44:04:01.5 -- not a known variable star
06:07:02.46 +48:02:59.7 -- not a known variable star
06:07:24.15 +50:24:29.1 -- not a known variable star
06:07:54.33 +45:58:50.4 -- not a known variable star
06:08:55.89 +40:54:29.6 -- not a known variable star
06:09:22.20 +49:25:25.9 -- not a known variable star
06:09:37.27 +50:22:55.0 -- not a known variable star
06:09:51.89 +46:34:26.9 -- a known variable star
06:10:07.33 +44:01:21.5 -- not a known variable star
06:10:43.27 +49:06:27.8 -- not a known variable star
06:10:45.09 +48:16:56.9 -- not a known variable star
06:11:46.84 +45:23:10.4 -- not a known variable star
06:12:04.54 +50:30:16.5 -- not a known variable star
06:12:57.22 +46:18:37.3 -- a known variable star
06:13:25.89 +44:01:20.8 -- a known variable star
06:14:06.03 +47:38:25.0 -- not a known variable star
06:14:47.66 +44:30:39.3 -- not a known variable star
06:15:04.64 +44:49:06.3 -- a known variable star
06:16:35.99 +46:36:14.4 -- not a known variable star
06:17:25.77 +46:39:38.7 -- not a known variable star
06:17:46.27 +40:58:41.6 -- not a known variable star
06:18:41.62 +42:18:28.3 -- not a known variable star
06:21:42.80 +40:56:53.7 -- not a known variable star
06:21:46.53 +48:41:42.7 -- not a known variable star
06:24:43.89 +43:30:23.1 -- not a known variable star
06:26:19.91 +41:59:10.9 -- not a known variable star
06:28:34.71 +47:18:32.1 -- not a known variable star
06:31:45.58 +48:30:01.6 -- a known variable star
06:34:07.99 +45:28:14.4 -- not a known variable star
06:34:52.65 +41:24:32.0 -- not a known variable star
06:35:53.18 +43:17:38.7 -- not a known variable star
06:36:59.28 +48:07:03.5 -- not a known variable star
06:37:22.56 +44:41:37.7 -- not a known variable star
06:40:23.63 +49:50:43.3 -- not a known variable star
06:43:51.18 +48:22:27.1 -- not a known variable star
06:48:54.16 +49:20:22.7 -- not a known variable star
Found 159 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
181 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 181 (excluding asteroids and hot pixels, 159 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461146.65137969 -observatory V36
00:08:04.98 -01:58:33.2 Mercury (0.0mag)
03:09:23.04 +17:54:52.1 Venus (-3.9mag)
00:18:16.25 +00:54:43.7 Mars (1.2mag)
07:12:41.95 +22:46:07.2 Jupiter (-2.1mag)
00:29:14.92 +00:49:24.1 Saturn (0.9mag)
03:47:43.72 +19:47:34.7 Uranus (5.8mag)
00:10:51.60 -00:15:14.8 Neptune (7.8mag)
20:33:45.67 -22:52:36.2 Pluto (14.5mag)
00:22:13.40 +04:47:32.2 Moon (-8.5mag)
-rw-r--r-- 1 apache apache 361 Apr 15 22:46 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461146.65137969:
07:12:44.21 +22:46:04.9 Io (5.8mag)
07:12:48.05 +22:45:56.7 Europa (5.9mag)
07:12:58.63 +22:45:28.3 Ganymede (5.4mag)
07:13:17.33 +22:44:54.8 Callisto (6.6mag)
07:16:01.80 +22:33:40.5 Himalia (15.3mag)
07:12:39.15 +22:46:11.7 Thebe (16.2mag)
07:16:13.38 +23:03:52.8 Elara (17.3mag)
07:11:35.46 +23:26:02.8 Pasiphae (17.4mag)
07:21:01.46 +22:44:09.4 Carme (18.5mag)
00:29:15.31 +00:49:50.5 Titan (8.8mag)
00:29:13.58 +00:49:27.9 Rhea (10.1mag)
00:28:54.67 +00:49:32.1 Iapetus (11.5mag)
00:29:22.70 +00:49:44.4 Hyperion (14.8mag)
00:30:51.70 +00:58:11.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 15 22:46 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.65137969:
15:39:09.13 -16:21:25.2 JWST
13:44:26.07 +55:28:36.5 Chandra
07:56:34.95 -36:38:08.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 15 22:46 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.65137969 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:03.95 -28:47:15.9 13.9mag P/2010 H2 (Vales)
05:06:50.58 -69:39:16.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:28.71 +31:26:18.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:25.28 +10:33:56.2 17.6mag C/2021 G2 (ATLAS)
23:10:15.86 +29:14:05.4 17.1mag C/2022 E2 (ATLAS)
04:29:24.73 +26:02:33.2 16.0mag C/2022 N2 (PANSTARRS)
09:03:27.14 +32:01:07.1 16.2mag C/2022 QE78 (ATLAS)
08:31:05.77 -00:08:13.5 17.3mag C/2022 R6 (PANSTARRS)
18:53:41.77 +18:32:42.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:37.57 -11:31:09.8 17.5mag P/2023 B1 (PANSTARRS)
09:07:33.92 -11:51:32.1 17.6mag C/2023 F3 (ATLAS)
21:54:22.05 +62:54:54.4 17.5mag C/2023 H5 (Lemmon)
19:19:04.18 -03:44:05.9 14.1mag C/2023 R1 (PANSTARRS)
21:32:14.39 +85:55:56.2 17.8mag C/2023 X2 (Lemmon)
06:17:58.02 +63:30:44.5 17.2mag C/2024 A1 (ATLAS)
05:13:36.01 +18:21:31.5 11.1mag C/2024 E1 (Wierzchos)
16:19:10.79 +06:24:55.0 17.4mag C/2024 G6 (ATLAS)
20:20:51.27 +15:18:55.4 14.6mag C/2024 J3 (ATLAS)
03:26:30.22 -22:21:44.9 16.3mag C/2024 T5 (ATLAS)
05:16:50.41 +45:15:12.6 17.7mag C/2025 J1 (Borisov)
13:38:12.47 +45:35:22.0 15.2mag C/2025 L1 (ATLAS)
03:25:30.80 -26:14:07.1 17.8mag C/2025 Q3 (ATLAS)
23:44:44.85 +18:33:40.6 8.5mag C/2025 R3 (PANSTARRS)
12:54:03.19 +03:01:19.2 17.4mag C/2025 Y1 (ATLAS)
03:29:10.62 +02:36:13.9 13.3mag C/2026 A1 (MAPS)
00:00:00.56 +37:14:50.4 14.6mag C/2026 B2 (Sun-Gao)
18:43:13.83 -09:42:39.4 11.8mag 10P/Tempel
15:00:06.25 +03:11:37.1 14.0mag 24P/Schaumasse
11:02:45.73 -01:31:16.6 15.7mag 29P/Schwassmann-Wachmann
18:01:00.47 -09:36:16.2 17.9mag 40P/Vaisala
10:37:33.50 -04:05:12.6 16.9mag 43P/Wolf-Harrington
01:48:54.43 +17:30:48.4 17.2mag 47P/Ashbrook-Jackson
07:11:02.56 +36:58:49.7 17.0mag 63P/Wild
23:29:15.00 -11:25:57.5 15.7mag 65P/Gunn
04:03:39.13 +21:18:26.0 15.9mag 76P/West-Kohoutek-Ikemura
01:05:54.52 +08:15:30.5 14.3mag 78P/Gehrels
23:03:27.69 -09:20:46.9 14.6mag 88P/Howell
02:10:49.64 +20:40:58.0 15.1mag 93P/Lovas
04:55:05.24 +32:17:45.4 16.2mag 123P/West-Hartley
08:28:32.37 +38:17:29.4 16.2mag 124P/Mrkos
02:33:26.93 +14:23:12.9 16.4mag 128P/Shoemaker-Holt
02:47:50.00 +14:30:42.2 17.5mag 131P/Mueller
01:26:57.52 +13:17:27.5 10.6mag 141P/Machholz
01:35:52.02 +04:55:50.2 10.6mag 141P-A/Machholz
00:21:05.33 +00:50:03.6 12.8mag 141P-D/Machholz
02:06:12.51 +06:41:23.1 17.8mag 141P-I/Machholz
01:02:47.97 -01:26:58.7 15.1mag 162P/SidingSpring
14:51:09.97 -00:03:08.3 17.7mag 210P/Christensen
21:39:17.09 -11:24:43.3 17.6mag 218P/LINEAR
17:16:36.42 -13:54:54.0 16.1mag 235P/LINEAR
05:34:48.49 +34:42:37.8 16.8mag 240P/NEAT
07:38:34.06 -05:09:02.7 17.7mag 242P/Spahr
22:17:17.18 -20:56:23.1 17.9mag 260P/McNaught
01:58:29.83 +20:29:55.6 18.0mag 295P/LINEAR
15:42:35.28 +07:00:01.9 17.5mag 391P/Kowalski
07:34:15.21 +21:21:59.6 17.7mag 450P/LONEOS
05:36:05.44 +45:01:26.0 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 15 22:46 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 15 22:46 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:52:32.558 +54:28:28.21 AT 2026iyo 2026-04-07.50 19.8736
12:10:51.131 -15:24:05.80 AT 2026iyn 2026-04-07.49 19.8
10:03:32.464 +00:47:38.92 AT 2026iym 2026-04-09.07 21.7842
09:57:46.577 +02:32:54.17 AT 2026iyl 2026-04-09.07 21.1159
12:09:21.288 -14:20:40.69 AT 2026iyk 2026-02-24.42 19.0617
11:32:15.323 +26:34:23.97 AT 2026iyi 2026-04-07.27 20.0038
08:41:36.643 +41:14:51.53 AT 2026iyh 2026-03-18.28 20.5874
11:10:47.748 -02:27:00.61 AT 2026iyg 2026-04-07.26 20.12
11:41:25.329 -11:32:16.55 AT 2026iyf 2026-04-07.25 20.8489
09:58:35.594 -17:44:37.57 AT 2026iye 2026-04-08.19 19.4848
07:48:08.582 +43:35:35.35 AT 2026iyd 2026-04-05.16 19.8382
11:13:43.729 +21:50:31.84 AT 2026iyc 2026-04-05.18 20.0005
08:02:45.458 +40:40:22.73 AT 2026iyb 2026-03-26.18 20.4831
13:05:52.496 +64:22:32.75 AT 2026iya 2026-03-08.94 19.29
05:15:26.423 -02:54:24.54 AT 2026ixz 2026-04-08.14 19.1905
14:04:24.118 +43:40:15.80 AT 2026ixt 2026-04-08.93 19.74
13:12:41.279 +38:05:24.08 AT 2026ixs 2026-04-08.93 20.18
13:21:56.843 -04:01:33.33 AT 2026ixr 2026-04-08.90 19.48
12:04:52.343 +69:44:57.80 AT 2026ixq 2026-04-08.89 19.03
21:31:46.671 +04:33:36.35 AT 2026ixp 2026-04-08.51 19.1697
-rw-r--r-- 1 apache apache 30K Apr 15 22:46 tns_transients_list.txt
