This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 10.2076 2461140.7076 11.88 05:16:30.03 +45:55:23.4
162.63086 4.49650 galactic Aur Second-epoch detections are separated by 2.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 211733267699198720 | 05:16:29.94 +45:55:15.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 211733267699198720,2461140.7076,11.88,0.05,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
Large-amplitude variable Gaia DR2 211733267699198720 20260410.2076 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.5401+44.9189,2461140.7076,13.85,0.05,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 J085.5401+44.9189 20260410.2076 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,2461140.7076,13.73,0.05,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 20260410.2076 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,2461140.7076,13.78,0.05,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
target 20260410.2076 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
target,2461140.7076,13.57,0.05,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 20260410.2076 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.6416+46.4725,2461140.7076,13.56,0.05,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 J087.6416+46.4725 20260410.2076 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.51,0.05,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 20260410.2076 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
target,2461140.7076,13.62,0.05,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 20260410.2076 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.5836+50.3884,2461140.7076,13.65,0.05,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 J092.5836+50.3884 20260410.2076 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,2461140.7076,13.56,0.05,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
target 20260410.2076 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 J087.5522+44.8128,2461140.7076,13.65,0.05,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 J087.5522+44.8128 20260410.2076 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,2461140.7076,13.50,0.05,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 20260410.2076 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6295+48.7004,2461140.7076,13.36,0.05,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
ATO J084.6295+48.7004 20260410.2076 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,2461140.7076,13.50,0.05,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 20260410.2076 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196107828779642752,2461140.7076,13.41,0.05,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 196107828779642752 20260410.2076 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,2461140.7076,13.49,0.05,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 20260410.2076 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,2461140.7076,13.38,0.05,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
target 20260410.2076 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.52,0.05,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 20260410.2076 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.10,0.05,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 20260410.2076 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.38,0.05,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
target 20260410.2076 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4559+44.4571,2461140.7076,13.19,0.05,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 J091.4559+44.4571 20260410.2076 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.12,0.05,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 20260410.2076 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208115904504557696,2461140.7076,13.01,0.05,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 208115904504557696 20260410.2076 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211950176426827264,2461140.7076,12.95,0.05,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
Gaia DR3 211950176426827264 20260410.2076 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197875298016710784,2461140.7076,12.93,0.05,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 197875298016710784 20260410.2076 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.55,0.05,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 20260410.2076 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0152+49.4731,2461140.7076,12.67,0.05,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
ATO J082.0152+49.4731 20260410.2076 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.5902+47.3234,2461140.7076,12.62,0.05,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
ATO J080.5902+47.3234 20260410.2076 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194881259137151872,2461140.7076,12.66,0.05,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
Gaia DR3 194881259137151872 20260410.2076 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6215+41.2425,2461140.7076,12.58,0.05,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 J084.6215+41.2425 20260410.2076 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.52,0.05,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 20260410.2076 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208280796888874240,2461140.7076,12.54,0.05,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 208280796888874240 20260410.2076 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
target,2461140.7076,12.44,0.05,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 20260410.2076 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.51,0.05,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 20260410.2076 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.2350+47.3510,2461140.7076,12.12,0.05,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 J086.2350+47.3510 20260410.2076 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963145561432116096,2461140.7076,11.94,0.05,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 963145561432116096 20260410.2076 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208124288279006336,2461140.7076,10.39,0.05,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 208124288279006336 20260410.2076 10.39CV 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
STARE aur0 543,2461140.7076,9.78,0.05,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
STARE aur0 543 20260410.2076 9.78CV 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 J084.3456+46.8139,2461140.7076,10.24,0.05,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 J084.3456+46.8139 20260410.2076 10.24CV 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 968776980814493824,2461140.7076,11.00,0.05,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 968776980814493824 20260410.2076 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461140.7076,11.21,0.05,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 20260410.2076 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
Gaia DR3 963538701262091904,2461140.7076,11.40,0.05,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 963538701262091904 20260410.2076 11.40CV 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 196564783236506368,2461140.7076,11.76,0.05,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 196564783236506368 20260410.2076 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 J095.4408+46.7822,2461140.7076,11.95,0.05,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
ATO J095.4408+46.7822 20260410.2076 11.95CV 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 J085.0114+50.0334,2461140.7076,11.91,0.05,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
ATO J085.0114+50.0334 20260410.2076 11.91CV 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 J088.9926+46.7105,2461140.7076,11.95,0.05,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
ATO J088.9926+46.7105 20260410.2076 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195701735329132160,2461140.7076,11.97,0.05,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
Gaia DR3 195701735329132160 20260410.2076 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1320+46.5774,2461140.7076,12.16,0.05,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 J089.1320+46.5774 20260410.2076 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211566141928805888,2461140.7076,12.18,0.05,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 20260410.2076 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197968717848571264,2461140.7076,12.05,0.05,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 197968717848571264 20260410.2076 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.0101+43.3293,2461140.7076,12.18,0.05,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 20260410.2076 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196143842081588352,2461140.7076,12.24,0.05,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
Gaia DR3 196143842081588352 20260410.2076 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3861+47.5396,2461140.7076,12.36,0.05,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
ATO J090.3861+47.5396 20260410.2076 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196796848908972032,2461140.7076,12.19,0.05,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
Gaia DR3 196796848908972032 20260410.2076 12.19CV 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 212655861031529216,2461140.7076,12.34,0.05,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 212655861031529216 20260410.2076 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 207586386576089984,2461140.7076,12.32,0.05,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 207586386576089984 20260410.2076 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.41,0.05,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
target 20260410.2076 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.0097+46.6828,2461140.7076,12.61,0.05,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
ATO J092.0097+46.6828 20260410.2076 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 J082.6900+43.4677,2461140.7076,12.60,0.05,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 J082.6900+43.4677 20260410.2076 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054610.24+465447.5,2461140.7076,12.57,0.05,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
ASASSN-V J054610.24+465447.5 20260410.2076 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0489+43.4659,2461140.7076,12.63,0.05,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 20260410.2076 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
Gaia DR3 967525667862574848,2461140.7076,12.74,0.05,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
Gaia DR3 967525667862574848 20260410.2076 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
ATO J083.8963+44.2568,2461140.7076,12.64,0.05,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 J083.8963+44.2568 20260410.2076 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.7165+46.8534,2461140.7076,12.71,0.05,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 J092.7165+46.8534 20260410.2076 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
target,2461140.7076,12.62,0.05,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
target 20260410.2076 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
target,2461140.7076,12.62,0.05,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
target 20260410.2076 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 958053585643972736,2461140.7076,12.97,0.05,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
Gaia DR3 958053585643972736 20260410.2076 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6086+42.9942,2461140.7076,12.68,0.05,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 J084.6086+42.9942 20260410.2076 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196601268981151360,2461140.7076,12.81,0.05,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
Gaia DR3 196601268981151360 20260410.2076 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 J084.9230+50.9576,2461140.7076,12.86,0.05,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 J084.9230+50.9576 20260410.2076 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.8867+42.5604,2461140.7076,12.72,0.05,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 J081.8867+42.5604 20260410.2076 12.72CV 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 211485843219678720,2461140.7076,12.79,0.05,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 211485843219678720 20260410.2076 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3023+47.5982,2461140.7076,12.89,0.05,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 J090.3023+47.5982 20260410.2076 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.77,0.05,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 20260410.2076 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.2234+48.7629,2461140.7076,12.85,0.05,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 20260410.2076 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
target,2461140.7076,12.85,0.05,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
target 20260410.2076 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
ZTF J053838.70+415545.6,2461140.7076,12.91,0.05,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
ZTF J053838.70+415545.6 20260410.2076 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461140.7076,12.80,0.05,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 J084.3195+44.0466 20260410.2076 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 192624786395334400,2461140.7076,12.81,0.05,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
Gaia DR3 192624786395334400 20260410.2076 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
Gaia DR3 966448253843543808,2461140.7076,13.17,0.05,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 966448253843543808 20260410.2076 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.84,0.05,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
target 20260410.2076 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968835396666764416,2461140.7076,12.99,0.05,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
Gaia DR3 968835396666764416 20260410.2076 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
ATO J082.6786+45.4850,2461140.7076,12.92,0.05,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 J082.6786+45.4850 20260410.2076 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207620613173739776,2461140.7076,12.73,0.05,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 207620613173739776 20260410.2076 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3774+41.9686,2461140.7076,12.99,0.05,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
ATO J093.3774+41.9686 20260410.2076 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 197388553666998656,2461140.7076,12.93,0.05,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 197388553666998656 20260410.2076 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3627+42.0135,2461140.7076,12.85,0.05,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 J084.3627+42.0135 20260410.2076 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
target,2461140.7076,13.12,0.05,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 20260410.2076 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.02,0.05,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 20260410.2076 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
target,2461140.7076,13.06,0.05,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
target 20260410.2076 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.00,0.05,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
target 20260410.2076 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195441288512899328,2461140.7076,12.92,0.05,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 195441288512899328 20260410.2076 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053001.72+474541.1,2461140.7076,13.03,0.05,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
ASASSN-V J053001.72+474541.1 20260410.2076 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1606+41.4155,2461140.7076,12.94,0.05,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
ATO J089.1606+41.4155 20260410.2076 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212612842640667008,2461140.7076,13.02,0.05,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
Gaia DR3 212612842640667008 20260410.2076 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
ZTF J051728.60+465934.4,2461140.7076,13.00,0.05,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
ZTF J051728.60+465934.4 20260410.2076 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.7154+50.4902,2461140.7076,12.96,0.05,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
ATO J080.7154+50.4902 20260410.2076 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,12.98,0.05,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 20260410.2076 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197673090956515200,2461140.7076,13.15,0.05,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 197673090956515200 20260410.2076 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211651594597874816,2461140.7076,13.19,0.05,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
Gaia DR3 211651594597874816 20260410.2076 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461140.7076,13.01,0.05,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 20260410.2076 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196540181664371200,2461140.7076,13.16,0.05,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 196540181664371200 20260410.2076 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 J083.5567+44.2856,2461140.7076,13.16,0.05,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 J083.5567+44.2856 20260410.2076 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 J086.4626+44.3866,2461140.7076,13.12,0.05,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 J086.4626+44.3866 20260410.2076 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197725867514471040,2461140.7076,13.16,0.05,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 197725867514471040 20260410.2076 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
ASASSN-V J053745.20+455814.5,2461140.7076,13.20,0.05,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 20260410.2076 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461140.7076,13.15,0.05,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 20260410.2076 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.22,0.05,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 20260410.2076 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.2593+47.3690,2461140.7076,13.18,0.05,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 J090.2593+47.3690 20260410.2076 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461140.7076,13.15,0.05,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 20260410.2076 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2314+46.6988,2461140.7076,13.27,0.05,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 J089.2314+46.6988 20260410.2076 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210103654024515072,2461140.7076,13.34,0.05,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 210103654024515072 20260410.2076 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963235824465355264,2461140.7076,13.28,0.05,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 963235824465355264 20260410.2076 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.1689+45.0683,2461140.7076,13.48,0.05,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 J093.1689+45.0683 20260410.2076 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193611907321181312,2461140.7076,13.37,0.05,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
Gaia DR3 193611907321181312 20260410.2076 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.21,0.05,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 20260410.2076 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.8193+42.1946,2461140.7076,13.30,0.05,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 J090.8193+42.1946 20260410.2076 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
target,2461140.7076,13.23,0.05,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 20260410.2076 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.7520+48.5869,2461140.7076,13.25,0.05,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
ATO J080.7520+48.5869 20260410.2076 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 197183292886359680,2461140.7076,13.31,0.05,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 20260410.2076 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.62,0.05,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 20260410.2076 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.7517+50.8577,2461140.7076,13.40,0.05,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
ATO J084.7517+50.8577 20260410.2076 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.3234+48.2792,2461140.7076,13.44,0.05,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 20260410.2076 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 J089.5381+48.6224,2461140.7076,13.36,0.05,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
ATO J089.5381+48.6224 20260410.2076 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
ATO J084.4674+50.9186,2461140.7076,13.60,0.05,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 J084.4674+50.9186 20260410.2076 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,2461140.7076,13.60,0.05,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
target 20260410.2076 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,2461140.7076,13.39,0.05,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 20260410.2076 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 963597147177904512,2461140.7076,13.50,0.05,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 963597147177904512 20260410.2076 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.3958+50.3918,2461140.7076,13.47,0.05,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 20260410.2076 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.60,0.05,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
target 20260410.2076 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 J083.3038+45.6310,2461140.7076,13.38,0.05,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 J083.3038+45.6310 20260410.2076 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962506603441468928,2461140.7076,13.40,0.05,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 962506603441468928 20260410.2076 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.2329+47.2571,2461140.7076,13.38,0.05,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 J082.2329+47.2571 20260410.2076 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.1386+40.7534,2461140.7076,13.62,0.05,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
ATO J097.1386+40.7534 20260410.2076 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 196695041004261120,2461140.7076,13.57,0.05,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
Gaia DR3 196695041004261120 20260410.2076 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,2461140.7076,13.64,0.05,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
target 20260410.2076 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9787+49.1928,2461140.7076,13.74,0.05,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
ATO J100.9787+49.1928 20260410.2076 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3650+48.6832,2461140.7076,13.53,0.05,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 J083.3650+48.6832 20260410.2076 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196564851955979392,2461140.7076,13.47,0.05,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 196564851955979392 20260410.2076 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197898903157490048,2461140.7076,13.71,0.05,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 197898903157490048 20260410.2076 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,2461140.7076,13.72,0.05,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 20260410.2076 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 J092.3081+48.2172,2461140.7076,13.90,0.05,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 J092.3081+48.2172 20260410.2076 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461140.7076,13.88,0.05,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 20260410.2076 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8999+48.2678,2461140.7076,13.77,0.05,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
ATO J089.8999+48.2678 20260410.2076 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 198142646844130816,2461140.7076,13.72,0.05,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 198142646844130816 20260410.2076 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,2461140.7076,13.87,0.05,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 20260410.2076 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
target,2461140.7076,13.75,0.05,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 20260410.2076 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.70,0.05,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
target 20260410.2076 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
Gaia DR3 214611613043441792,2461140.7076,13.80,0.05,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
Gaia DR3 214611613043441792 20260410.2076 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,2461140.7076,13.63,0.05,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 20260410.2076 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209617876043883136,2461140.7076,13.77,0.05,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 209617876043883136 20260410.2076 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
ATO J091.7998+46.6816,2461140.7076,13.75,0.05,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 J091.7998+46.6816 20260410.2076 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.97,0.05,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 20260410.2076 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
target,2461140.7076,13.79,0.05,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
target 20260410.2076 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,2461140.7076,14.07,0.05,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 20260410.2076 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7076,13.84,0.05,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
target 20260410.2076 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
target,2461140.7076,13.91,0.05,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 20260410.2076 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
Gaia DR3 210886506303538048,2461140.7076,13.74,0.05,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
Gaia DR3 210886506303538048 20260410.2076 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
## 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: 2461140.70797014 10.04.2026 04:59:18.620 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23031
Objects passed selection criteria: 23006
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 20563.5
Average stars matched: 20115.5 (97.8214 %)
Memory usage VmPeak: 126872 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:49:12 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: 2461140.70797014 10.04.2026 04:59:18.620 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 463
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: 99 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): 163299
Objects passed selection criteria: 162935
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: 152753
Average stars matched: 147990 (96.8814 %)
Memory usage VmPeak: 1934676 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:52:43 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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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: 2461140.70728206
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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:17.161 +45:57:56.73
Angular distance between the image centers 0.0957 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:18.709 +45:58:25.98
Angular distance between the image centers 0.0964 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 06:00:17.161 +45:57:56.73
Second-epoch second image center 06:00:18.709 +45:58:25.98
Angular distance between the image centers 0.00928 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.iWoyNjgBiE
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.tLcFweSqTg
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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits &> /tmp/tmp.P6x7rosmJ0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits &> /tmp/tmp.hecU9APZ9l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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 15 candidate transients before the final filtering. (Hard limit: 3000)
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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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
15.0 mag. fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
15.0 mag. fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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.iWoyNjgBiE (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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.tLcFweSqTg (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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.P6x7rosmJ0 (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1237, passed=17070
Got 17070 stars (including 15802 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 17070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 16656 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 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 16655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 16655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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.hecU9APZ9l (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1232, passed=17129
Got 17129 stars (including 15871 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 17129 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 925 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 16745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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: 925 matched stars entering correct_measured_positions(), 16744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 16744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31663.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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 31501_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31501_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:25.85 +42:08:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.257 195187640625510784 079.60810998508 +42.14645632842 12.2162 11.8228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31502_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31502_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:46.22 +43:34:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31506_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31506_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:33:58.53 +49:58:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31547_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31547_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:27.45 +44:52:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.42, MAG_FAINT_SEARCH_LIMIT=11.40)GAIADR2_OUTPUT=# 1.264 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31575_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31575_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:43.42 +44:59:10.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31582_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31582_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:14:59.10 +46:47:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31595_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31595_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:44:52.49 +49:21:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31600_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31600_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:42.20 +43:22:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31662_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31662_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:42.89 +43:37:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31663_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 31663_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 31666_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31666_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:21.22 +50:18:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31704_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31704_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:19.77 +43:42:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.591 962654114094673536 092.83250592858 +43.71246754807 12.2907 11.8607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31726_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 31726_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:57.47 +43:47:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.776 961201758017019648 091.48936574688 +43.78965603324 12.2410 11.5458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:01.79 +50:29:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 17s
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 ####
05:16:30.03 +45:55:23.4
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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:17.161 +45:57:56.73
Angular distance between the image centers 0.0957 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:18.709 +45:58:25.98
Angular distance between the image centers 0.0964 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 06:00:17.161 +45:57:56.73
Second-epoch second image center 06:00:18.709 +45:58:25.98
Angular distance between the image centers 0.00928 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.U7uqNZi7lX
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.07uNCi9FJe
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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits &> /tmp/tmp.KNl7AcHG2v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits &> /tmp/tmp.lss01TBfzg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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 441 candidate transients before the final filtering. (Hard limit: 3000)
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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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
14.1 mag. fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
14.1 mag. fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (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.U7uqNZi7lX (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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.07uNCi9FJe (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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.KNl7AcHG2v (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=11472, passed=137629
Got 137629 stars (including 125938 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 137629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 135345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 135347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 135348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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.lss01TBfzg (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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=11305, passed=135926
Got 135926 stars (including 124388 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 135926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 132862 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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 132862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 132863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/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_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-58-19_20.00sec_-4.90C_LIGHTs_0066.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-10_CI_Aur-02-Q1b1x1_000020_TTUQ1b1x1_913_Hc2LdMvr/wcs_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out195200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197680.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 218s
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: 98s
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Considering the candidate 195200_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195200_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195205_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:02:46.31 +43:11:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.595 961310236008163584 090.69277451352 +43.18682756288 14.6315 14.0764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195222_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195222_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195244_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195244_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195246_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195246_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195249_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195249_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:12.80 +50:13:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.490 970415910271615232 091.05354351434 +50.22491000811 14.7079 14.1289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195251_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195251_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:49.38 +48:57:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.608 214015750756237440 083.70511604589 +48.96077313812 14.5731 13.7425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195255_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195255_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195257_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195257_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195258_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195258_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:29.13 +50:48:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.360 214608142708363904 087.62182050965 +50.80269248900 14.4520 13.7482 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195272_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195272_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195279_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195279_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:23.89 +41:07:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.949 192615921585878144 085.59992109105 +41.11642898370 14.2796 13.5889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195282_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195282_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:55.93 +48:15:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.320 210368292729975680 087.73351448248 +48.25943769764 14.1467 13.3080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195283_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195283_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195295_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195295_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:24.38 +50:20:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.305 211569852780732288 089.35236411573 +50.33418129791 14.5141 13.8996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195296_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:19.73 +49:30:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.429 211320950835685760 088.58240636243 +49.50098562142 14.3802 13.6966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:15.70 +49:01:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195305_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195305_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:12.82 +44:18:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.760 197083787085249024 085.55409525404 +44.30225092962 14.2648 13.6264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195311_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195311_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195315_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:36.76 +47:42:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.152 969703667255081728 090.90347088593 +47.71592073831 14.4357 13.8490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:27.47 +43:48:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.904 195611163059241088 083.61450272044 +43.80372310162 14.1797 13.5453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195328_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195328_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:04.16 +50:05:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.025 211551161082978432 088.51749029006 +50.09856694290 14.2592 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195336_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195336_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195338_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195338_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195342_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195342_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195343_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195343_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:03.47 +49:21:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195344_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195344_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195348_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195348_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:51.94 +50:23:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.789 214201774379210496 086.46695159388 +50.39635992125 14.3866 13.7258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195350_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:13.66 +44:13:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.110 207776400226843264 082.55694286433 +44.22264101995 14.0720 13.1129 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195356_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195356_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:57.70 +42:35:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195358_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195358_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195363_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195363_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:35:00.24 +50:18:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195376_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:45.86 +42:29:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.146 194717603702894848 083.19152712637 +42.49977592488 13.8863 13.3275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195377_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:32.94 +42:15:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:47.29 +45:03:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.749 208070485227161856 081.94772240108 +45.06093054383 13.6714 13.1299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195390_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195390_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:44.42 +50:48:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195392_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195392_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:29.59 +50:53:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.966 213907242702848896 082.62243045009 +50.88366608650 14.1676 13.6215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195393_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195393_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:24:03.90 +44:40:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.760 959256898041674880 096.01653084857 +44.67501473517 13.9280 13.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195395_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:57.88 +44:00:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195401_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:37.82 +42:19:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.022 960842806127020160 090.90720582013 +42.32964201630 13.9868 13.3718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195403_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195403_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:09.81 +43:57:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.604 195756676550349952 082.29129462561 +43.95432762591 13.9174 13.3689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195405_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195405_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195406_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195406_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195407_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195407_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195408_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195408_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:34.61 +43:43:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.575 195694966460793216 082.64506841991 +43.73265983499 13.9964 13.1690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195411_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:03.92 +44:42:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195412_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:55.15 +49:27:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195417_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195417_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:35.78 +48:01:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.752 212371289380254336 081.89926390564 +48.01699616597 13.7292 13.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195418_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195418_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:45.70 +44:06:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.548 193513501030173056 088.44062354178 +44.11243952429 13.8894 13.2651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195420_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:26.95 +42:40:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195426_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195426_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:41.94 +45:46:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.944 208912848572994048 081.67479168285 +45.77804489760 13.7646 13.1770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:32.24 +44:46:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.018 208507438020791168 079.63499485094 +44.76780532452 13.8388 12.9895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195441_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195441_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:44.22 +50:59:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.051 215225007387998592 085.93446186108 +50.98390711228 13.5660 12.9195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195443_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195443_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:27.83 +47:36:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195445_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195445_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195447_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195447_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:59.55 +44:37:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.647 207708127426423808 080.74876747824 +44.62546209328 13.6319 12.8108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195448_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195448_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:37.83 +42:12:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195449_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195449_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:50.61 +41:27:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195452_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195452_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195459_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195459_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:14.79 +49:31:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195461_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195461_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:33:19.95 +49:59:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195462_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195462_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:55.52 +50:56:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195463_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195463_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:59.23 +46:26:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.710 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195466_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195466_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195472_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195472_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:47.35 +42:06:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195477_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195477_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:44.36 +43:14:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195479_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195479_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:16:43.02 +44:42:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.459 962379987803965568 094.17937221668 +44.71614908613 13.4420 12.7072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195481_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195481_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:29.01 +41:11:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.469 194185886752655232 081.62042213918 +41.19197008772 13.3302 12.7961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195482_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195482_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:53.70 +50:04:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195483_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:23.04 +46:50:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195487_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195487_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:16:36.24 +44:32:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.507 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195488_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195488_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:28.45 +45:37:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.235 963105979013594368 091.36854584114 +45.63049033177 13.4451 13.0245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195490_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195490_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195493_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195493_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:01.68 +46:28:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.330 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195496_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195496_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:00.06 +43:23:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195497_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195497_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:24.69 +42:28:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195501_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195501_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:57.65 +44:20:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.156 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195503_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195503_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195505_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195505_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195507_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195507_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:14.21 +42:05:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195510_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195510_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:47.74 +43:12:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195512_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195512_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:20:13.24 +43:38:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.685 961773886316261504 095.05528574915 +43.64410819835 12.5992 12.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:23.63 +49:53:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195516_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195516_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:34.63 +45:32:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.961 963062342146066432 090.14422902412 +45.53343101528 12.7393 12.0346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195517_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195517_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:38.26 +48:20:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.158 210370418736729472 087.90946632657 +48.33580450234 12.7164 12.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195518_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195518_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:28.82 +47:01:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.404 210567300037906816 083.87064439310 +47.03086736119 12.1803 11.3066 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 195520_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195520_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:42.16 +43:39:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.120 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195522_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195522_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:45.97 +43:34:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195523_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195523_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:43.96 +41:42:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195526_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195526_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195527_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195527_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195610_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195610_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:44:52.51 +49:21:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195613_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195613_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:27.55 +42:19:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.14, MAG_FAINT_SEARCH_LIMIT=11.12)GAIADR2_OUTPUT=# 0.333 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195625_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195625_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195626_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195626_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:08:02.93 +48:43:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195693_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195693_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:42.89 +43:37:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195701_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195701_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195716_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195716_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:34.52 +48:44:35.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195740_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195740_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195749_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195749_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:48.08 +43:44:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195766_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195766_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195787_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195787_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:31.42 +50:41:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.373 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195792_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195792_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:46:26.52 +47:55:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.293 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195802_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195802_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:01.46 +41:06:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195808_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195808_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:36.55 +40:59:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195824_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195824_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:36:59.32 +48:07:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.079 967332673508208256 099.24717563820 +48.11763216666 12.6763 12.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195829_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195829_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:19:04.21 +47:21:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.641 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195831_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195831_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:06:21.41 +48:46:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.992 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195874_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195874_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:02:11.25 +46:42:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.984 963599006899237888 090.54702525212 +46.71599679132 12.7537 11.9893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195883_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195883_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195903_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195903_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195906_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195906_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195917_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195917_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:23.55 +48:55:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195920_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195920_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:46.65 +44:43:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.778 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195927_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195927_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:51.84 +42:57:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195934_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195934_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:07.54 +44:53:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.530 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195944_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195944_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195948_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195948_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:50.21 +44:39:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.380 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 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 195957_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195957_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:08.20 +51:03:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195961_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195961_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:48.35 +46:57:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.710 198029362786762880 089.20161100133 +46.96494369065 12.8922 12.0517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195973_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195973_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 195974_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195974_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:09.70 +47:19:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.624 212316245079377280 081.04053074053 +47.31751152611 12.7573 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195989_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 195989_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:03.10 +42:12:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195996_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 195996_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196008_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196008_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:52.20 +46:46:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196009_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196009_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196017_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196017_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:40.93 +44:01:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.268 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196020_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196020_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:11.10 +43:58:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196033_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196033_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196036_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196036_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:56.62 +46:08:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196037_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196037_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:39.84 +47:54:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.730 212586660519063680 080.66597215012 +47.91400751652 13.0455 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196038_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196038_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:44.73 +46:30:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196046_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196046_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196050_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196050_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:51.32 +41:14:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.341 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196052_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196052_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196060_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196060_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196066_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196066_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:58.22 +50:54:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196072_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196072_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:25.89 +48:47:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196091_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196091_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:06.00 +41:55:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.594 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196094_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196094_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:13.62 +42:56:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196095_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196095_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:43.96 +41:18:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.281 194505771619147776 082.18314538158 +41.30272918703 13.1352 12.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196096_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196096_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:46.08 +45:53:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.825 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196099_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196099_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:16.18 +46:04:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.554 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196102_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196102_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:10.15 +50:14:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196113_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196113_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196114_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196114_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:52.72 +44:00:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.037 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196118_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196118_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196119_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196119_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:40.63 +41:28:15.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196124_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196124_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:28.73 +45:52:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.752 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196127_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196127_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196134_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196134_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:02.46 +49:49:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.371 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196140_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196140_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:32.60 +43:42:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.345 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196142_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196142_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:44.02 +42:26:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196145_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196145_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:45.31 +50:03:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.012 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196158_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196158_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:17.74 +42:18:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196159_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196159_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:12.07 +45:24:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.502 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196160_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196160_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:16:31.70 +45:54:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196178_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196178_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:34.78 +46:23:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196179_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196179_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:51.86 +41:10:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196182_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196182_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:04.63 +42:17:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196186_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196186_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:01.06 +47:29:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.196 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196194_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196194_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:31:06.81 +48:10:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196196_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196196_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:50.42 +42:19:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196207_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196207_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:01:04.65 +50:00:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.059 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196211_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196211_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:09.24 +43:26:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196223_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196223_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:14.30 +50:00:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196243_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196243_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:44.76 +44:40:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.504 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196258_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196258_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:06.24 +45:12:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196261_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196261_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:02.10 +42:43:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.157 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196265_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196265_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:48.26 +48:58:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196268_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196268_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:23.46 +42:09:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196270_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196270_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:37.93 +41:51:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.047 192902481803698688 084.65904102262 +41.85839798429 13.5174 12.7370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196275_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196275_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:41.13 +48:21:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196278_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196278_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:23.91 +50:13:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.887 261808836861057408 080.84799330687 +50.23144343721 13.3252 12.3513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196280_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196280_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196282_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196282_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:17.95 +43:17:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196288_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196288_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:42.33 +45:31:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196289_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:07.14 +41:10:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196295_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196295_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:48.19 +42:30:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196300_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196300_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196301_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196301_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:03.67 +49:32:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196305_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196305_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:19.76 +47:53:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.313 212214338394071808 080.33245046079 +47.89648151556 13.1631 12.2515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196308_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196308_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:58.89 +43:48:27.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196310_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196310_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196312_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196312_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:59.42 +46:40:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196325_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196325_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:15.05 +40:57:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:03.07 +41:43:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.246 960200034204636544 093.01317175941 +41.73174612260 13.5765 12.8505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196328_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196328_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:02:48.85 +43:13:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196332_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196332_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196341_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196341_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:38:13.82 +40:38:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196343_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196343_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:15.77 +41:56:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.399 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196349_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196349_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:06.56 +44:51:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 0.969 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196359_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196359_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:42.73 +47:53:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.452 212586385641158912 080.67776024297 +47.89856027064 13.3715 12.5283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196362_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196362_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196364_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196364_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:41.51 +50:41:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.342 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196375_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196375_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:47.43 +47:00:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.240 212303050943149440 080.69756548932 +47.01475255644 13.7614 13.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:13.92 +47:43:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.904 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196381_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196381_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:15:16.35 +42:09:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196391_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196391_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196393_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196393_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:22.06 +42:59:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.101 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 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 196394_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196394_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:30.24 +41:38:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196397_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196397_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:46.46 +46:04:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.284 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196400_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196400_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:31.27 +47:51:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.440 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196403_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196403_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:27.55 +46:35:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196406_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:57.51 +43:06:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.146 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196408_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196408_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:02.34 +46:44:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196409_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196409_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196413_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196413_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196417_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196417_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:31.10 +44:15:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.000 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196420_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196420_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:08:21.83 +42:58:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196430_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196430_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:59.21 +43:51:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196431_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196431_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196432_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196432_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:18.52 +44:01:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.882 197062106090089600 084.82750509630 +44.02700003359 13.7838 13.2144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196433_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196433_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196435_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196435_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:40.43 +42:51:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196468_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196468_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:21.20 +45:06:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.976 196674081564004352 089.83869973985 +45.11475185016 13.8009 13.0282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:21.74 +47:52:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196479_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:46:39.79 +43:21:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196482_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196482_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:53.95 +46:06:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196487_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196487_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196493_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196493_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196495_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196495_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:32.60 +41:57:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196499_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196499_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:27.90 +47:51:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196504_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196504_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196506_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196506_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:24:18.10 +43:22:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196513_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196513_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:50.45 +49:49:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196515_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:30.37 +43:50:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.961 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196519_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196519_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196523_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196523_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:20.01 +49:14:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196525_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196525_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:45.47 +45:22:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196531_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196531_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:33.89 +45:29:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196537_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196537_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196538_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196538_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196543_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196543_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:37.74 +43:07:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196549_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196549_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:58.01 +43:42:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.176 207515987770326784 079.74275755653 +43.70229955072 13.6619 12.7892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196565_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196565_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:49.70 +49:26:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196571_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196571_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196575_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196575_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:50.53 +44:16:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196579_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196579_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:22:29.82 +44:29:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.996 962230007546590208 095.62484427373 +44.49039250040 13.9307 13.4207 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196580_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196580_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:28.93 +46:52:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.062 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196581_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196581_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196584_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196584_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:24.80 +49:14:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196590_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196590_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:28.66 +41:25:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196592_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196592_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196593_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196593_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196594_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196594_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:20:02.71 +46:37:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196595_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196595_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:05.50 +48:44:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196599_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196599_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:21.23 +42:41:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196610_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196610_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196614_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196614_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:49.13 +51:04:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196618_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196618_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196622_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196622_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196626_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196626_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:13.59 +46:47:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196629_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196629_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196633_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196633_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:23:09.80 +49:10:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.597 970593653198168064 095.79099454777 +49.16629137386 14.1385 13.6837 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196634_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196634_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:50.68 +48:07:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.636 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196638_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196638_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:18.15 +46:15:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196647_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196647_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196649_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196649_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196652_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196652_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:01.97 +50:28:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196654_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196654_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:56.68 +47:43:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.232 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196658_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196658_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196661_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196661_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:44.93 +47:30:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.681 968792721871861888 093.18747696802 +47.51186298846 14.0070 13.4569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196668_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196668_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:21.14 +42:50:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196671_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196671_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196673_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196673_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:43.73 +50:12:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196679_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196679_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:56.41 +50:48:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.041 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196695_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196695_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:32.05 +48:16:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.459 212436955138189696 083.38339755979 +48.28147147774 13.9515 13.4567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196696_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196696_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196703_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196703_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:03.54 +46:04:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196708_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196708_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196710_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196710_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:44.72 +49:34:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.457 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 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 196714_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196714_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:44.15 +47:47:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.574 212218358483551616 079.93457606840 +47.79294561915 13.8506 12.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196718_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196718_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:38.76 +47:49:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.120 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196722_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196722_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:24.79 +44:48:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.854 208086290707268608 081.10372106703 +44.80994290569 13.9169 13.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196726_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196726_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:25.38 +42:20:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.550 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196730_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196730_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196738_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196738_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:18.67 +47:12:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.186 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 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 196742_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196742_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196750_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196750_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:09.19 +45:30:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.606 208175935264007040 082.78821481371 +45.51453490536 14.1469 13.5285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196751_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196751_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:28.26 +42:41:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196752_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196752_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:57.06 +41:37:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.772 192277649962098688 087.98771623166 +41.62337032686 13.8897 13.1157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196758_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196758_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196763_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196763_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:41.24 +44:16:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196769_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196769_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:13.58 +49:41:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.354 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 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 196772_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196772_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:05.30 +47:54:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.606 212973070136674176 079.77194120619 +47.91030574196 14.0911 13.4071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196783_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196783_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:18.31 +44:16:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.577 207789005953568000 082.07681950966 +44.26697163248 13.7769 12.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196784_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:48.17 +42:30:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196786_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196786_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196788_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196788_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:32.33 +48:50:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.848 212734441750616576 082.38435419683 +48.83832739506 14.0076 13.1565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196794_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196794_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:58.70 +46:09:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196805_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196805_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196812_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196812_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:37.57 +42:21:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196815_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196815_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196816_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196816_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196818_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196818_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:24.16 +41:41:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196825_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196825_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:00.76 +49:05:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.610 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196826_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196826_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196828_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196828_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196831_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196831_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196840_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196840_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196846_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196846_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:35.82 +50:10:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196850_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196850_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196854_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196854_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:15.36 +42:06:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196861_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196861_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:51.78 +45:03:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.226 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 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 196866_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196866_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:20.07 +50:12:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.126 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196869_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196869_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196883_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196883_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:34.17 +51:09:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.990 261966208758451968 082.39187092852 +51.16684242895 14.0311 13.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196885_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196885_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:36:58.93 +49:45:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196887_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196887_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196896_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196896_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196903_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196903_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:56.51 +50:32:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.490 215106157052998784 084.23555796130 +50.54292433083 14.0941 13.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196912_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196912_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196914_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196914_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:36.96 +50:13:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196922_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196922_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:41.70 +49:06:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196937_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196937_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196944_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196944_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:11.16 +46:03:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.614 197523351216767360 086.79557643499 +46.05504755708 14.1430 13.2999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196947_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196947_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:47.45 +45:58:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196960_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196960_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:07.16 +47:47:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.885 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196972_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196972_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 196977_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196977_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:59.83 +47:35:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.326 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196980_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196980_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:55.47 +45:00:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196981_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196981_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:06.36 +46:08:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196983_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 196983_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196987_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196987_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:42:04.52 +49:39:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.601 991157299479352960 100.51871738467 +49.66107312699 14.5771 14.0745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196993_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 196993_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:48.57 +48:50:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197012_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197012_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197021_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197021_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197030_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197030_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197039_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197039_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197043_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197043_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:07.94 +44:47:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197046_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197046_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197053_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197053_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197058_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197058_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197072_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197072_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197074_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197074_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:19:35.34 +50:11:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.722 970984628365709056 094.89747534126 +50.19355523935 14.5323 13.7967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197079_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197079_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197086_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197086_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197122_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197122_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197132_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197132_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:48.93 +46:10:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.781 208974588724407424 081.95398429282 +46.17604659977 13.9532 13.0798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197135_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197135_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197139_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197139_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197161_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197161_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197205_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197205_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:22.48 +44:11:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.157 195815053746718848 083.84380070058 +44.19055680741 14.4729 13.9262 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197219_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197219_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197220_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197220_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197225_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197225_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:17.25 +47:02:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197237_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197237_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197242_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197242_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:12.41 +46:37:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.167 211860707967806848 080.55175356227 +46.62856539187 14.2153 13.3047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197245_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197245_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:27.01 +46:08:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.289 208267160368960000 083.61303104489 +46.14235709444 14.3490 13.4590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197253_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197253_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:16:58.55 +49:51:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.693 970868462385389056 094.24396130289 +49.85688684092 14.5664 13.9458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197285_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197285_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197288_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197288_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197297_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197297_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:37:06.31 +46:32:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.667 965646331909197184 099.27649342221 +46.53487281291 14.5882 13.8863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197304_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197307_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197307_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:03.85 +49:39:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.350 214110446194930560 086.26624730253 +49.65684395412 14.4453 13.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197318_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197318_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:06.90 +45:48:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.093 208904292998072448 082.02997456906 +45.80198770002 14.4267 13.4532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197321_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197324_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197324_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197325_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197325_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:16.71 +42:10:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 0.473 192939040564836096 085.06976204516 +42.18288895315 14.4139 13.8388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197326_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197326_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:11.31 +47:42:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.456 210275246558703488 087.29796699323 +47.71064786462 14.3323 13.6937 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197327_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:29.03 +42:28:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.912 193169113373091712 087.37164333181 +42.46913586159 14.6077 13.7720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197332_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197332_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:00.01 +50:38:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.940 262056506150513408 079.99963124658 +50.63450696523 14.3638 13.4517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197336_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197336_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:38:49.85 +50:12:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.536 991934791639334400 099.70787976546 +50.21437148436 14.6564 14.1037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197369_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197369_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:36.57 +48:08:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.068 212457845858919424 082.40318324799 +48.13661800230 14.5949 14.0236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197372_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197372_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:47.09 +47:20:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.291 209357978983188864 082.69669623066 +47.34752735043 14.4460 13.8493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197376_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197376_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:47:42.82 +49:56:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.537 991036185697897728 101.92835542094 +49.94024514629 14.7017 14.1827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197386_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197386_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:00.29 +46:40:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.780 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197388_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197388_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197402_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197402_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197409_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197409_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:17.39 +48:38:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.777 210393066101070976 087.82317447496 +48.64291830688 14.5406 13.7761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197416_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197416_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:48.32 +45:07:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.043 197224829514684544 086.95075015175 +45.11662289086 14.6563 13.7935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197424_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197424_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197432_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197432_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:44.44 +47:23:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.170 209368561782176768 082.43555143845 +47.39801569514 14.7644 13.9755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197440_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197440_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:28.96 +50:29:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.006 214425902952905984 085.62098238470 +50.49186118074 14.4616 13.6596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197441_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197441_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197443_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197443_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197446_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197446_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:19.94 +49:43:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.189 970294311157627264 091.33310339506 +49.72928098849 14.6509 14.0910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197457_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:11.41 +44:24:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.148 196614123820820224 088.79795499937 +44.41032398753 14.8452 14.1751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197474_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197478_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197478_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:35.03 +50:10:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.318 213632021198277376 082.89588145654 +50.18223210576 14.3987 13.5553 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#
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Considering the candidate 197480_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197480_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:52.82 +49:47:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.808 211450521408874880 087.97050814910 +49.78983950430 14.8977 14.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197488_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197488_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197491_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197503_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197503_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:19.80 +47:40:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.346 210096197961186944 088.08316586129 +47.66913839098 14.5637 13.9920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197505_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197505_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197509_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197509_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:47.11 +44:57:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.038 963015853420168704 090.19662718302 +44.95080844354 14.7279 14.0293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197513_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197513_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:14.22 +49:59:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.049 215054720524924160 083.56013394319 +49.98538785788 14.7954 14.0341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197514_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197518_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197518_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:09.27 +47:01:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.191 209676665556055552 086.78937106254 +47.02441587096 14.6563 13.7357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197533_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197533_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:39.63 +50:33:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.728 215188792223848320 084.91587514206 +50.55655498757 14.4739 13.6267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197535_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197535_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:01:32.43 +48:06:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.312 969772008774566528 090.38550220391 +48.10359754765 14.5671 13.9081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197547_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197547_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:25.82 +49:33:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.416 970708517803708672 096.35776094841 +49.55031825811 14.7467 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197551_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197551_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:02:57.93 +46:27:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.669 963568667249950592 090.74225943407 +46.46168855447 13.3894 11.9357 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197557_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197557_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 197559_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197559_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:50.24 +47:10:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.870 969438788032333696 092.95967878636 +47.18180398358 14.6455 13.9349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197560_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197560_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197579_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197579_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:09.16 +43:47:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.801 961928058462191616 093.03817496808 +43.78363871250 14.7390 14.0677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197608_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197608_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:07:04.30 +43:37:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.245 961196230395290240 091.76798080454 +43.62192236236 14.7744 14.3135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197621_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197621_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:21.62 +42:55:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.691 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197644_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197644_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:48.80 +47:50:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.484 210849603944817664 083.95385514517 +47.83981062777 14.4444 13.5806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197646_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197646_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197651_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197651_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197654_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197654_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:02.02 +42:01:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197664_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197664_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197672_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 197672_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:45.85 +45:04:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.572 197224455852769280 086.94120466206 +45.08119300612 14.6628 13.9871 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197680_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 197680_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:14:59.08 +46:47:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:41:12.80 +44:09:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:56.95 +44:41:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:24.02 +48:22:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:29.87 +43:44:35.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:44.15 +47:37:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-09_23-59-18_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:01.77 +50:29:26.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 326s
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 ####
05:16:30.03 +45:55:23.4
05:42:09.50 +44:55:07.6
05:58:04.17 +45:09:36.8
05:56:52.45 +43:51:22.0
05:47:36.73 +49:32:40.0
05:50:38.25 +46:28:15.5
06:08:37.44 +46:49:53.7
05:28:49.53 +50:42:03.9
06:10:20.57 +50:23:14.0
06:03:40.60 +43:42:53.4
05:50:10.38 +44:48:35.6
06:18:02.57 +43:28:05.7
05:38:30.99 +48:42:01.0
05:58:08.64 +46:59:24.3
05:46:17.11 +43:28:20.1
06:08:52.42 +45:50:38.2
06:04:49.69 +49:11:46.5
06:07:50.11 +44:09:42.8
06:13:09.37 +41:15:40.5
05:57:30.26 +45:13:25.4
06:05:45.84 +44:27:21.0
05:57:51.23 +50:11:53.6
05:27:02.79 +45:02:38.3
05:21:49.21 +47:17:19.9
05:59:43.69 +47:14:06.7
05:25:14.10 +41:06:55.9
05:28:04.11 +49:28:30.4
05:22:21.88 +47:19:34.6
05:19:23.19 +41:14:44.0
05:38:27.40 +41:13:51.5
05:27:16.26 +45:33:34.1
05:33:14.91 +46:13:29.6
05:37:52.69 +48:05:35.3
05:15:02.08 +48:43:56.1
05:44:58.24 +47:20:57.3
06:01:39.51 +45:44:14.4
05:28:11.13 +45:21:59.2
05:17:56.34 +41:11:54.4
05:37:22.96 +46:49:18.6
06:15:16.65 +47:16:52.8
05:25:37.72 +45:40:57.2
06:04:44.11 +46:34:52.1
05:49:28.95 +44:16:20.5
06:21:48.17 +46:46:32.1
05:40:02.77 +50:02:05.9
05:55:58.22 +46:42:37.7
05:25:48.83 +43:15:19.0
05:56:34.24 +46:35:08.3
05:57:40.02 +50:14:50.7
05:48:45.97 +46:35:02.1
05:48:04.13 +43:19:50.7
05:43:47.29 +43:32:42.8
06:01:32.40 +47:32:26.8
05:53:06.77 +44:56:01.9
05:28:01.40 +48:15:01.0
05:18:48.27 +44:06:46.5
06:26:19.88 +41:59:11.5
06:08:02.31 +46:40:58.7
05:30:45.56 +43:28:04.9
05:46:10.02 +46:54:48.4
05:28:11.78 +43:27:55.9
06:25:48.93 +48:15:43.8
05:35:35.19 +44:15:17.4
06:10:50.08 +46:51:09.0
05:27:26.09 +44:48:51.9
05:27:51.11 +42:20:26.7
06:38:26.78 +42:30:58.6
05:38:24.40 +42:59:49.4
05:52:15.69 +44:44:13.9
05:39:41.60 +50:57:37.8
05:27:30.92 +42:33:45.2
05:48:23.15 +49:46:58.3
06:01:16.80 +47:35:46.1
05:44:39.73 +43:57:56.0
05:32:56.23 +48:45:35.6
05:39:19.11 +44:01:56.2
05:38:35.55 +41:55:50.0
05:37:16.34 +44:02:46.7
05:40:57.33 +41:07:46.0
06:43:05.33 +46:46:43.5
05:19:09.85 +44:39:54.8
06:13:33.63 +48:03:17.9
05:30:42.54 +45:28:58.6
05:20:50.92 +44:04:38.2
06:13:29.81 +41:58:07.5
05:37:19.55 +44:51:38.7
05:37:28.44 +42:00:46.4
06:26:29.80 +49:54:11.2
06:00:04.49 +45:58:33.7
05:58:48.93 +42:14:42.8
05:57:12.05 +42:33:33.9
05:27:26.99 +42:42:33.2
05:30:04.77 +47:45:35.5
05:56:40.80 +41:24:47.0
05:23:51.98 +48:16:07.6
05:17:29.44 +46:59:13.2
05:22:55.68 +50:29:43.4
05:23:23.68 +46:46:23.1
05:49:15.66 +45:41:17.3
05:56:40.48 +50:40:59.4
05:50:26.50 +44:11:29.7
05:48:18.90 +43:50:50.5
05:34:15.76 +44:17:06.7
05:45:50.35 +44:23:02.1
05:52:11.32 +46:15:48.5
05:37:41.44 +45:58:10.3
05:50:28.71 +44:11:35.6
05:28:03.28 +44:53:44.5
06:01:02.19 +47:22:16.2
05:34:19.01 +44:27:44.5
05:56:58.08 +46:41:30.1
05:50:48.69 +47:35:40.3
06:10:00.20 +45:32:43.7
06:12:43.11 +45:04:27.1
05:55:36.73 +44:15:36.6
05:37:52.45 +43:02:35.7
06:03:15.22 +42:11:14.6
05:56:28.21 +47:43:40.0
05:22:57.29 +48:35:35.7
05:43:59.79 +44:30:09.7
06:25:47.82 +49:52:45.8
05:39:00.96 +50:51:38.3
06:05:14.75 +48:16:59.1
05:58:09.64 +48:37:13.4
05:37:51.95 +50:55:07.4
06:20:59.78 +43:39:47.6
05:46:44.67 +43:22:55.2
06:03:02.81 +46:44:00.0
06:09:37.13 +50:22:56.3
05:39:52.15 +43:03:15.8
05:33:11.80 +45:37:49.2
06:18:00.66 +45:11:50.4
05:29:00.41 +47:15:55.2
06:28:33.70 +40:45:39.6
05:55:34.73 +44:58:58.0
05:52:08.41 +49:39:13.3
06:43:53.28 +49:12:00.2
05:33:25.87 +48:41:08.5
05:49:28.09 +44:17:59.6
05:47:47.72 +46:06:01.3
05:32:48.26 +50:40:06.1
06:09:09.96 +48:13:10.7
05:53:50.66 +46:42:31.0
05:59:31.96 +48:16:11.9
05:57:28.83 +47:42:23.4
06:24:00.40 +46:40:56.7
05:37:18.89 +50:58:17.1
05:34:45.13 +46:34:30.1
05:49:56.65 +50:48:52.9
05:26:51.26 +45:04:16.6
05:45:22.45 +46:37:59.4
06:07:09.27 +46:41:04.8
05:50:02.96 +50:00:53.2
05:34:10.02 +44:23:50.9
05:57:58.55 +48:05:37.9
05:49:00.05 +44:11:43.5
05:55:21.21 +44:40:00.2
05:39:27.06 +48:10:53.4
########### 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 ####
05:16:30.03 +45:55:23.4
05:42:09.50 +44:55:07.6
05:58:04.17 +45:09:36.8
05:56:52.45 +43:51:22.0
05:47:36.73 +49:32:40.0
05:50:38.25 +46:28:15.5
06:08:37.44 +46:49:53.7
05:28:49.53 +50:42:03.9
06:10:20.57 +50:23:14.0
06:03:40.60 +43:42:53.4
05:50:10.38 +44:48:35.6
06:18:02.57 +43:28:05.7
05:38:30.99 +48:42:01.0
05:58:08.64 +46:59:24.3
05:46:17.11 +43:28:20.1
06:08:52.42 +45:50:38.2
06:04:49.69 +49:11:46.5
06:07:50.11 +44:09:42.8
06:13:09.37 +41:15:40.5
05:57:30.26 +45:13:25.4
06:05:45.84 +44:27:21.0
05:57:51.23 +50:11:53.6
05:27:02.79 +45:02:38.3
05:21:49.21 +47:17:19.9
05:59:43.69 +47:14:06.7
05:25:14.10 +41:06:55.9
05:28:04.11 +49:28:30.4
05:22:21.88 +47:19:34.6
05:19:23.19 +41:14:44.0
05:38:27.40 +41:13:51.5
05:27:16.26 +45:33:34.1
05:33:14.91 +46:13:29.6
05:37:52.69 +48:05:35.3
05:15:02.08 +48:43:56.1
05:44:58.24 +47:20:57.3
06:01:39.51 +45:44:14.4
05:28:11.13 +45:21:59.2
05:17:56.34 +41:11:54.4
05:37:22.96 +46:49:18.6
06:15:16.65 +47:16:52.8
05:25:37.72 +45:40:57.2
06:04:44.11 +46:34:52.1
05:49:28.95 +44:16:20.5
06:21:48.17 +46:46:32.1
05:40:02.77 +50:02:05.9
05:55:58.22 +46:42:37.7
05:25:48.83 +43:15:19.0
05:56:34.24 +46:35:08.3
05:57:40.02 +50:14:50.7
05:48:45.97 +46:35:02.1
05:48:04.13 +43:19:50.7
05:43:47.29 +43:32:42.8
06:01:32.40 +47:32:26.8
05:53:06.77 +44:56:01.9
05:28:01.40 +48:15:01.0
05:18:48.27 +44:06:46.5
06:26:19.88 +41:59:11.5
06:08:02.31 +46:40:58.7
05:30:45.56 +43:28:04.9
05:46:10.02 +46:54:48.4
05:28:11.78 +43:27:55.9
06:25:48.93 +48:15:43.8
05:35:35.19 +44:15:17.4
06:10:50.08 +46:51:09.0
05:27:26.09 +44:48:51.9
05:27:51.11 +42:20:26.7
06:38:26.78 +42:30:58.6
05:38:24.40 +42:59:49.4
05:52:15.69 +44:44:13.9
05:39:41.60 +50:57:37.8
05:27:30.92 +42:33:45.2
05:48:23.15 +49:46:58.3
06:01:16.80 +47:35:46.1
05:44:39.73 +43:57:56.0
05:32:56.23 +48:45:35.6
05:39:19.11 +44:01:56.2
05:38:35.55 +41:55:50.0
05:37:16.34 +44:02:46.7
05:40:57.33 +41:07:46.0
06:43:05.33 +46:46:43.5
05:19:09.85 +44:39:54.8
06:13:33.63 +48:03:17.9
05:30:42.54 +45:28:58.6
05:20:50.92 +44:04:38.2
06:13:29.81 +41:58:07.5
05:37:19.55 +44:51:38.7
05:37:28.44 +42:00:46.4
06:26:29.80 +49:54:11.2
06:00:04.49 +45:58:33.7
05:58:48.93 +42:14:42.8
05:57:12.05 +42:33:33.9
05:27:26.99 +42:42:33.2
05:30:04.77 +47:45:35.5
05:56:40.80 +41:24:47.0
05:23:51.98 +48:16:07.6
05:17:29.44 +46:59:13.2
05:22:55.68 +50:29:43.4
05:23:23.68 +46:46:23.1
05:49:15.66 +45:41:17.3
05:56:40.48 +50:40:59.4
05:50:26.50 +44:11:29.7
05:48:18.90 +43:50:50.5
05:34:15.76 +44:17:06.7
05:45:50.35 +44:23:02.1
05:52:11.32 +46:15:48.5
05:37:41.44 +45:58:10.3
05:50:28.71 +44:11:35.6
05:28:03.28 +44:53:44.5
06:01:02.19 +47:22:16.2
05:34:19.01 +44:27:44.5
05:56:58.08 +46:41:30.1
05:50:48.69 +47:35:40.3
06:10:00.20 +45:32:43.7
06:12:43.11 +45:04:27.1
05:55:36.73 +44:15:36.6
05:37:52.45 +43:02:35.7
06:03:15.22 +42:11:14.6
05:56:28.21 +47:43:40.0
05:22:57.29 +48:35:35.7
05:43:59.79 +44:30:09.7
06:25:47.82 +49:52:45.8
05:39:00.96 +50:51:38.3
06:05:14.75 +48:16:59.1
05:58:09.64 +48:37:13.4
05:37:51.95 +50:55:07.4
06:20:59.78 +43:39:47.6
05:46:44.67 +43:22:55.2
06:03:02.81 +46:44:00.0
06:09:37.13 +50:22:56.3
05:39:52.15 +43:03:15.8
05:33:11.80 +45:37:49.2
06:18:00.66 +45:11:50.4
05:29:00.41 +47:15:55.2
06:28:33.70 +40:45:39.6
05:55:34.73 +44:58:58.0
05:52:08.41 +49:39:13.3
06:43:53.28 +49:12:00.2
05:33:25.87 +48:41:08.5
05:49:28.09 +44:17:59.6
05:47:47.72 +46:06:01.3
05:32:48.26 +50:40:06.1
06:09:09.96 +48:13:10.7
05:53:50.66 +46:42:31.0
05:59:31.96 +48:16:11.9
05:57:28.83 +47:42:23.4
06:24:00.40 +46:40:56.7
05:37:18.89 +50:58:17.1
05:34:45.13 +46:34:30.1
05:49:56.65 +50:48:52.9
05:26:51.26 +45:04:16.6
05:45:22.45 +46:37:59.4
06:07:09.27 +46:41:04.8
05:50:02.96 +50:00:53.2
05:34:10.02 +44:23:50.9
05:57:58.55 +48:05:37.9
05:49:00.05 +44:11:43.5
05:55:21.21 +44:40:00.2
05:39:27.06 +48:10:53.4
###################################################################################
05:16:30.03 +45:55:23.4 -- not an asteroid (will add it to exclusion list)
05:42:09.50 +44:55:07.6 -- not an asteroid (will add it to exclusion list)
05:58:04.17 +45:09:36.8 -- not an asteroid (will add it to exclusion list)
05:56:52.45 +43:51:22.0 -- not an asteroid (will add it to exclusion list)
05:47:36.73 +49:32:40.0 -- not an asteroid (will add it to exclusion list)
05:50:38.25 +46:28:15.5 -- not an asteroid (will add it to exclusion list)
06:08:37.44 +46:49:53.7 -- not an asteroid (will add it to exclusion list)
05:28:49.53 +50:42:03.9 -- not an asteroid (will add it to exclusion list)
06:10:20.57 +50:23:14.0 -- not an asteroid (will add it to exclusion list)
06:03:40.60 +43:42:53.4 -- not an asteroid (will add it to exclusion list)
05:50:10.38 +44:48:35.6 -- not an asteroid (will add it to exclusion list)
06:18:02.57 +43:28:05.7 -- not an asteroid (will add it to exclusion list)
05:38:30.99 +48:42:01.0 -- not an asteroid (will add it to exclusion list)
05:58:08.64 +46:59:24.3 -- not an asteroid (will add it to exclusion list)
05:46:17.11 +43:28:20.1 -- not an asteroid (will add it to exclusion list)
06:08:52.42 +45:50:38.2 -- not an asteroid (will add it to exclusion list)
06:04:49.69 +49:11:46.5 -- not an asteroid (will add it to exclusion list)
06:07:50.11 +44:09:42.8 -- not an asteroid (will add it to exclusion list)
06:13:09.37 +41:15:40.5 -- not an asteroid (will add it to exclusion list)
05:57:30.26 +45:13:25.4 -- not an asteroid (will add it to exclusion list)
06:05:45.84 +44:27:21.0 -- not an asteroid (will add it to exclusion list)
05:57:51.23 +50:11:53.6 -- not an asteroid (will add it to exclusion list)
05:27:02.79 +45:02:38.3 -- not an asteroid (will add it to exclusion list)
05:21:49.21 +47:17:19.9 -- not an asteroid (will add it to exclusion list)
05:59:43.69 +47:14:06.7 -- not an asteroid (will add it to exclusion list)
05:25:14.10 +41:06:55.9 -- not an asteroid (will add it to exclusion list)
05:28:04.11 +49:28:30.4 -- not an asteroid (will add it to exclusion list)
05:22:21.88 +47:19:34.6 -- not an asteroid (will add it to exclusion list)
05:19:23.19 +41:14:44.0 -- not an asteroid (will add it to exclusion list)
05:38:27.40 +41:13:51.5 -- not an asteroid (will add it to exclusion list)
05:27:16.26 +45:33:34.1 -- not an asteroid (will add it to exclusion list)
05:33:14.91 +46:13:29.6 -- not an asteroid (will add it to exclusion list)
05:37:52.69 +48:05:35.3 -- not an asteroid (will add it to exclusion list)
05:15:02.08 +48:43:56.1 -- not an asteroid (will add it to exclusion list)
05:44:58.24 +47:20:57.3 -- not an asteroid (will add it to exclusion list)
06:01:39.51 +45:44:14.4 -- not an asteroid (will add it to exclusion list)
05:28:11.13 +45:21:59.2 -- not an asteroid (will add it to exclusion list)
05:17:56.34 +41:11:54.4 -- not an asteroid (will add it to exclusion list)
05:37:22.96 +46:49:18.6 -- not an asteroid (will add it to exclusion list)
06:15:16.65 +47:16:52.8 -- not an asteroid (will add it to exclusion list)
05:25:37.72 +45:40:57.2 -- not an asteroid (will add it to exclusion list)
06:04:44.11 +46:34:52.1 -- not an asteroid (will add it to exclusion list)
05:49:28.95 +44:16:20.5 -- not an asteroid (will add it to exclusion list)
06:21:48.17 +46:46:32.1 -- not an asteroid (will add it to exclusion list)
05:40:02.77 +50:02:05.9 -- not an asteroid (will add it to exclusion list)
05:55:58.22 +46:42:37.7 -- not an asteroid (will add it to exclusion list)
05:25:48.83 +43:15:19.0 -- not an asteroid (will add it to exclusion list)
05:56:34.24 +46:35:08.3 -- not an asteroid (will add it to exclusion list)
05:57:40.02 +50:14:50.7 -- not an asteroid (will add it to exclusion list)
05:48:45.97 +46:35:02.1 -- not an asteroid (will add it to exclusion list)
05:48:04.13 +43:19:50.7 -- not an asteroid (will add it to exclusion list)
05:43:47.29 +43:32:42.8 -- not an asteroid (will add it to exclusion list)
06:01:32.40 +47:32:26.8 -- not an asteroid (will add it to exclusion list)
05:53:06.77 +44:56:01.9 -- not an asteroid (will add it to exclusion list)
05:28:01.40 +48:15:01.0 -- not an asteroid (will add it to exclusion list)
05:18:48.27 +44:06:46.5 -- not an asteroid (will add it to exclusion list)
06:26:19.88 +41:59:11.5 -- not an asteroid (will add it to exclusion list)
06:08:02.31 +46:40:58.7 -- not an asteroid (will add it to exclusion list)
05:30:45.56 +43:28:04.9 -- not an asteroid (will add it to exclusion list)
05:46:10.02 +46:54:48.4 -- not an asteroid (will add it to exclusion list)
05:28:11.78 +43:27:55.9 -- not an asteroid (will add it to exclusion list)
06:25:48.93 +48:15:43.8 -- not an asteroid (will add it to exclusion list)
05:35:35.19 +44:15:17.4 -- not an asteroid (will add it to exclusion list)
06:10:50.08 +46:51:09.0 -- not an asteroid (will add it to exclusion list)
05:27:26.09 +44:48:51.9 -- not an asteroid (will add it to exclusion list)
05:27:51.11 +42:20:26.7 -- not an asteroid (will add it to exclusion list)
06:38:26.78 +42:30:58.6 -- not an asteroid (will add it to exclusion list)
05:38:24.40 +42:59:49.4 -- not an asteroid (will add it to exclusion list)
05:52:15.69 +44:44:13.9 -- not an asteroid (will add it to exclusion list)
05:39:41.60 +50:57:37.8 -- not an asteroid (will add it to exclusion list)
05:27:30.92 +42:33:45.2 -- not an asteroid (will add it to exclusion list)
05:48:23.15 +49:46:58.3 -- not an asteroid (will add it to exclusion list)
06:01:16.80 +47:35:46.1 -- not an asteroid (will add it to exclusion list)
05:44:39.73 +43:57:56.0 -- not an asteroid (will add it to exclusion list)
05:32:56.23 +48:45:35.6 -- not an asteroid (will add it to exclusion list)
05:39:19.11 +44:01:56.2 -- not an asteroid (will add it to exclusion list)
05:38:35.55 +41:55:50.0 -- not an asteroid (will add it to exclusion list)
05:37:16.34 +44:02:46.7 -- not an asteroid (will add it to exclusion list)
05:40:57.33 +41:07:46.0 -- not an asteroid (will add it to exclusion list)
06:43:05.33 +46:46:43.5 -- not an asteroid (will add it to exclusion list)
05:19:09.85 +44:39:54.8 -- not an asteroid (will add it to exclusion list)
06:13:33.63 +48:03:17.9 -- not an asteroid (will add it to exclusion list)
05:30:42.54 +45:28:58.6 -- not an asteroid (will add it to exclusion list)
05:20:50.92 +44:04:38.2 -- not an asteroid (will add it to exclusion list)
06:13:29.81 +41:58:07.5 -- not an asteroid (will add it to exclusion list)
05:37:19.55 +44:51:38.7 -- not an asteroid (will add it to exclusion list)
05:37:28.44 +42:00:46.4 -- not an asteroid (will add it to exclusion list)
06:26:29.80 +49:54:11.2 -- not an asteroid (will add it to exclusion list)
06:00:04.49 +45:58:33.7 -- not an asteroid (will add it to exclusion list)
05:58:48.93 +42:14:42.8 -- not an asteroid (will add it to exclusion list)
05:57:12.05 +42:33:33.9 -- not an asteroid (will add it to exclusion list)
05:27:26.99 +42:42:33.2 -- not an asteroid (will add it to exclusion list)
05:30:04.77 +47:45:35.5 -- not an asteroid (will add it to exclusion list)
05:56:40.80 +41:24:47.0 -- not an asteroid (will add it to exclusion list)
05:23:51.98 +48:16:07.6 -- not an asteroid (will add it to exclusion list)
05:17:29.44 +46:59:13.2 -- not an asteroid (will add it to exclusion list)
05:22:55.68 +50:29:43.4 -- not an asteroid (will add it to exclusion list)
05:23:23.68 +46:46:23.1 -- not an asteroid (will add it to exclusion list)
05:49:15.66 +45:41:17.3 -- not an asteroid (will add it to exclusion list)
05:56:40.48 +50:40:59.4 -- not an asteroid (will add it to exclusion list)
05:50:26.50 +44:11:29.7 -- not an asteroid (will add it to exclusion list)
05:48:18.90 +43:50:50.5 -- not an asteroid (will add it to exclusion list)
05:34:15.76 +44:17:06.7 -- not an asteroid (will add it to exclusion list)
05:45:50.35 +44:23:02.1 -- not an asteroid (will add it to exclusion list)
05:52:11.32 +46:15:48.5 -- not an asteroid (will add it to exclusion list)
05:37:41.44 +45:58:10.3 -- not an asteroid (will add it to exclusion list)
05:50:28.71 +44:11:35.6 -- not an asteroid (will add it to exclusion list)
05:28:03.28 +44:53:44.5 -- not an asteroid (will add it to exclusion list)
06:01:02.19 +47:22:16.2 -- not an asteroid (will add it to exclusion list)
05:34:19.01 +44:27:44.5 -- not an asteroid (will add it to exclusion list)
05:56:58.08 +46:41:30.1 -- not an asteroid (will add it to exclusion list)
05:50:48.69 +47:35:40.3 -- not an asteroid (will add it to exclusion list)
06:10:00.20 +45:32:43.7 -- not an asteroid (will add it to exclusion list)
06:12:43.11 +45:04:27.1 -- not an asteroid (will add it to exclusion list)
05:55:36.73 +44:15:36.6 -- not an asteroid (will add it to exclusion list)
05:37:52.45 +43:02:35.7 -- not an asteroid (will add it to exclusion list)
06:03:15.22 +42:11:14.6 -- not an asteroid (will add it to exclusion list)
05:56:28.21 +47:43:40.0 -- not an asteroid (will add it to exclusion list)
05:22:57.29 +48:35:35.7 -- not an asteroid (will add it to exclusion list)
05:43:59.79 +44:30:09.7 -- not an asteroid (will add it to exclusion list)
06:25:47.82 +49:52:45.8 -- not an asteroid (will add it to exclusion list)
05:39:00.96 +50:51:38.3 -- not an asteroid (will add it to exclusion list)
06:05:14.75 +48:16:59.1 -- not an asteroid (will add it to exclusion list)
05:58:09.64 +48:37:13.4 -- not an asteroid (will add it to exclusion list)
05:37:51.95 +50:55:07.4 -- not an asteroid (will add it to exclusion list)
06:20:59.78 +43:39:47.6 -- not an asteroid (will add it to exclusion list)
05:46:44.67 +43:22:55.2 -- not an asteroid (will add it to exclusion list)
06:03:02.81 +46:44:00.0 -- not an asteroid (will add it to exclusion list)
06:09:37.13 +50:22:56.3 -- not an asteroid (will add it to exclusion list)
05:39:52.15 +43:03:15.8 -- not an asteroid (will add it to exclusion list)
05:33:11.80 +45:37:49.2 -- not an asteroid (will add it to exclusion list)
06:18:00.66 +45:11:50.4 -- not an asteroid (will add it to exclusion list)
05:29:00.41 +47:15:55.2 -- not an asteroid (will add it to exclusion list)
06:28:33.70 +40:45:39.6 -- not an asteroid (will add it to exclusion list)
05:55:34.73 +44:58:58.0 -- not an asteroid (will add it to exclusion list)
05:52:08.41 +49:39:13.3 -- not an asteroid (will add it to exclusion list)
06:43:53.28 +49:12:00.2 -- not an asteroid (will add it to exclusion list)
05:33:25.87 +48:41:08.5 -- not an asteroid (will add it to exclusion list)
05:49:28.09 +44:17:59.6 -- not an asteroid (will add it to exclusion list)
05:47:47.72 +46:06:01.3 -- not an asteroid (will add it to exclusion list)
05:32:48.26 +50:40:06.1 -- not an asteroid (will add it to exclusion list)
06:09:09.96 +48:13:10.7 -- not an asteroid (will add it to exclusion list)
05:53:50.66 +46:42:31.0 -- not an asteroid (will add it to exclusion list)
05:59:31.96 +48:16:11.9 -- not an asteroid (will add it to exclusion list)
05:57:28.83 +47:42:23.4 -- not an asteroid (will add it to exclusion list)
06:24:00.40 +46:40:56.7 -- not an asteroid (will add it to exclusion list)
05:37:18.89 +50:58:17.1 -- not an asteroid (will add it to exclusion list)
05:34:45.13 +46:34:30.1 -- not an asteroid (will add it to exclusion list)
05:49:56.65 +50:48:52.9 -- not an asteroid (will add it to exclusion list)
05:26:51.26 +45:04:16.6 -- not an asteroid (will add it to exclusion list)
05:45:22.45 +46:37:59.4 -- not an asteroid (will add it to exclusion list)
06:07:09.27 +46:41:04.8 -- not an asteroid (will add it to exclusion list)
05:50:02.96 +50:00:53.2 -- not an asteroid (will add it to exclusion list)
05:34:10.02 +44:23:50.9 -- not an asteroid (will add it to exclusion list)
05:57:58.55 +48:05:37.9 -- not an asteroid (will add it to exclusion list)
05:49:00.05 +44:11:43.5 -- not an asteroid (will add it to exclusion list)
05:55:21.21 +44:40:00.2 -- not an asteroid (will add it to exclusion list)
05:39:27.06 +48:10:53.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:15:02.08 +48:43:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:30.03 +45:55:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.44 +46:59:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:56.34 +41:11:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:48.27 +44:06:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.85 +44:39:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:23.19 +41:14:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.92 +44:04:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:49.21 +47:17:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:21.88 +47:19:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:55.68 +50:29:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:57.29 +48:35:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:23.68 +46:46:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:51.98 +48:16:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:14.10 +41:06:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.72 +45:40:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:48.83 +43:15:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:51.26 +45:04:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:02.79 +45:02:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:16.26 +45:33:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.09 +44:48:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.99 +42:42:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:30.92 +42:33:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:51.11 +42:20:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.40 +48:15:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:03.28 +44:53:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.11 +49:28:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.13 +45:21:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.78 +43:27:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:49.53 +50:42:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:00.41 +47:15:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:04.77 +47:45:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:42.54 +45:28:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:45.56 +43:28:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:48.26 +50:40:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.23 +48:45:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:11.80 +45:37:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:14.91 +46:13:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:25.87 +48:41:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:10.02 +44:23:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.76 +44:17:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.01 +44:27:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:45.13 +46:34:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:35.19 +44:15:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.34 +44:02:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:18.89 +50:58:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.55 +44:51:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:22.96 +46:49:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:28.44 +42:00:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.44 +45:58:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:51.95 +50:55:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.45 +43:02:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.69 +48:05:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:24.40 +42:59:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.40 +41:13:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:30.99 +48:42:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:35.55 +41:55:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:00.96 +50:51:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.11 +44:01:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:27.06 +48:10:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:41.60 +50:57:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:52.15 +43:03:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.77 +50:02:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:57.33 +41:07:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:09.50 +44:55:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.29 +43:32:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:59.79 +44:30:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:39.73 +43:57:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:58.24 +47:20:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:22.45 +46:37:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.35 +44:23:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:10.02 +46:54:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:17.11 +43:28:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:44.67 +43:22:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:36.73 +49:32:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:47.72 +46:06:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.13 +43:19:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:18.90 +43:50:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.15 +49:46:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:45.97 +46:35:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:00.05 +44:11:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:15.66 +45:41:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.09 +44:17:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.95 +44:16:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:56.65 +50:48:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:02.96 +50:00:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.38 +44:48:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:26.50 +44:11:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.71 +44:11:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:38.25 +46:28:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:48.69 +47:35:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:08.41 +49:39:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:11.32 +46:15:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:15.69 +44:44:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.77 +44:56:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:50.66 +46:42:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:21.21 +44:40:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:34.73 +44:58:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:36.73 +44:15:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:58.22 +46:42:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:28.21 +47:43:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:34.24 +46:35:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:40.48 +50:40:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:40.80 +41:24:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:52.45 +43:51:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:58.08 +46:41:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.05 +42:33:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:28.83 +47:42:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:30.26 +45:13:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:40.02 +50:14:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:51.23 +50:11:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:58.55 +48:05:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:04.17 +45:09:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:08.64 +46:59:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.64 +48:37:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:48.93 +42:14:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:31.96 +48:16:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:43.69 +47:14:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:04.49 +45:58:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:02.19 +47:22:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.80 +47:35:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.40 +47:32:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:39.51 +45:44:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:02.81 +46:44:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:15.22 +42:11:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:40.60 +43:42:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:44.11 +46:34:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:49.69 +49:11:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:14.75 +48:16:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:45.84 +44:27:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:09.27 +46:41:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:50.11 +44:09:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:02.31 +46:40:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:37.44 +46:49:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:52.42 +45:50:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:09.96 +48:13:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:37.13 +50:22:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:00.20 +45:32:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:20.57 +50:23:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:50.08 +46:51:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:43.11 +45:04:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:09.37 +41:15:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.81 +41:58:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:33.63 +48:03:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:16.65 +47:16:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:00.66 +45:11:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:02.57 +43:28:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:59.78 +43:39:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.17 +46:46:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:00.40 +46:40:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:47.82 +49:52:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:48.93 +48:15:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.88 +41:59:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.80 +49:54:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:33.70 +40:45:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:26.78 +42:30:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:05.33 +46:46:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:53.28 +49:12:00.2 -- 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)
05:15:02.08 +48:43:56.1 -- not a known variable star
05:16:30.03 +45:55:23.4 -- not a known variable star
05:17:29.44 +46:59:13.2 -- a known variable star
05:17:56.34 +41:11:54.4 -- a known variable star
05:18:48.27 +44:06:46.5 -- not a known variable star
05:19:09.85 +44:39:54.8 -- not a known variable star
05:19:23.19 +41:14:44.0 -- a known variable star
05:20:50.92 +44:04:38.2 -- not a known variable star
05:21:49.21 +47:17:19.9 -- a known variable star
05:22:21.88 +47:19:34.6 -- not a known variable star
05:22:55.68 +50:29:43.4 -- not a known variable star
05:22:57.29 +48:35:35.7 -- not a known variable star
05:23:23.68 +46:46:23.1 -- not a known variable star
05:23:51.98 +48:16:07.6 -- not a known variable star
05:25:14.10 +41:06:55.9 -- not a known variable star
05:25:37.72 +45:40:57.2 -- not a known variable star
05:25:48.83 +43:15:19.0 -- a known variable star
05:26:51.26 +45:04:16.6 -- not a known variable star
05:27:02.79 +45:02:38.3 -- a known variable star
05:27:16.26 +45:33:34.1 -- not a known variable star
05:27:26.09 +44:48:51.9 -- not a known variable star
05:27:26.99 +42:42:33.2 -- not a known variable star
05:27:30.92 +42:33:45.2 -- not a known variable star
05:27:51.11 +42:20:26.7 -- not a known variable star
05:28:01.40 +48:15:01.0 -- a known variable star
05:28:03.28 +44:53:44.5 -- not a known variable star
05:28:04.11 +49:28:30.4 -- not a known variable star
05:28:11.13 +45:21:59.2 -- not a known variable star
05:28:11.78 +43:27:55.9 -- not a known variable star
05:28:49.53 +50:42:03.9 -- not a known variable star
05:29:00.41 +47:15:55.2 -- not a known variable star
05:30:04.77 +47:45:35.5 -- not a known variable star
05:30:42.54 +45:28:58.6 -- not a known variable star
05:30:45.56 +43:28:04.9 -- not a known variable star
05:32:48.26 +50:40:06.1 -- not a known variable star
05:32:56.23 +48:45:35.6 -- not a known variable star
05:33:11.80 +45:37:49.2 -- not a known variable star
05:33:14.91 +46:13:29.6 -- a known variable star
05:33:25.87 +48:41:08.5 -- not a known variable star
05:34:10.02 +44:23:50.9 -- not a known variable star
05:34:15.76 +44:17:06.7 -- not a known variable star
05:34:19.01 +44:27:44.5 -- not a known variable star
05:34:45.13 +46:34:30.1 -- not a known variable star
05:35:35.19 +44:15:17.4 -- not a known variable star
05:37:16.34 +44:02:46.7 -- not a known variable star
05:37:18.89 +50:58:17.1 -- not a known variable star
05:37:19.55 +44:51:38.7 -- not a known variable star
05:37:22.96 +46:49:18.6 -- not a known variable star
05:37:28.44 +42:00:46.4 -- not a known variable star
05:37:41.44 +45:58:10.3 -- not a known variable star
05:37:51.95 +50:55:07.4 -- not a known variable star
05:37:52.45 +43:02:35.7 -- not a known variable star
05:37:52.69 +48:05:35.3 -- not a known variable star
05:38:24.40 +42:59:49.4 -- not a known variable star
05:38:27.40 +41:13:51.5 -- not a known variable star
05:38:30.99 +48:42:01.0 -- not a known variable star
05:38:35.55 +41:55:50.0 -- not a known variable star
05:39:00.96 +50:51:38.3 -- not a known variable star
05:39:19.11 +44:01:56.2 -- not a known variable star
05:39:27.06 +48:10:53.4 -- not a known variable star
05:39:41.60 +50:57:37.8 -- not a known variable star
05:39:52.15 +43:03:15.8 -- not a known variable star
05:40:02.77 +50:02:05.9 -- not a known variable star
05:40:57.33 +41:07:46.0 -- a known variable star
05:42:09.50 +44:55:07.6 -- not a known variable star
05:43:47.29 +43:32:42.8 -- not a known variable star
05:43:59.79 +44:30:09.7 -- a known variable star
05:44:39.73 +43:57:56.0 -- not a known variable star
05:44:58.24 +47:20:57.3 -- not a known variable star
05:45:22.45 +46:37:59.4 -- not a known variable star
05:45:50.35 +44:23:02.1 -- not a known variable star
05:46:10.02 +46:54:48.4 -- a known variable star
05:46:17.11 +43:28:20.1 -- a known variable star
05:46:44.67 +43:22:55.2 -- not a known variable star
05:47:36.73 +49:32:40.0 -- not a known variable star
05:47:47.72 +46:06:01.3 -- not a known variable star
05:48:04.13 +43:19:50.7 -- not a known variable star
05:48:18.90 +43:50:50.5 -- a known variable star
05:48:23.15 +49:46:58.3 -- not a known variable star
05:48:45.97 +46:35:02.1 -- a known variable star
05:49:00.05 +44:11:43.5 -- not a known variable star
05:49:15.66 +45:41:17.3 -- not a known variable star
05:49:28.09 +44:17:59.6 -- a known variable star
05:49:28.95 +44:16:20.5 -- not a known variable star
05:49:56.65 +50:48:52.9 -- not a known variable star
05:50:02.96 +50:00:53.2 -- not a known variable star
05:50:10.38 +44:48:35.6 -- not a known variable star
05:50:26.50 +44:11:29.7 -- a known variable star
05:50:28.71 +44:11:35.6 -- a known variable star
05:50:38.25 +46:28:15.5 -- not a known variable star
05:50:48.69 +47:35:40.3 -- a known variable star
05:52:08.41 +49:39:13.3 -- not a known variable star
05:52:11.32 +46:15:48.5 -- not a known variable star
05:52:15.69 +44:44:13.9 -- not a known variable star
05:53:06.77 +44:56:01.9 -- not a known variable star
05:53:50.66 +46:42:31.0 -- not a known variable star
05:55:21.21 +44:40:00.2 -- not a known variable star
05:55:34.73 +44:58:58.0 -- not a known variable star
05:55:36.73 +44:15:36.6 -- a known variable star
05:55:58.22 +46:42:37.7 -- not a known variable star
05:56:28.21 +47:43:40.0 -- not a known variable star
05:56:34.24 +46:35:08.3 -- not a known variable star
05:56:40.48 +50:40:59.4 -- not a known variable star
05:56:40.80 +41:24:47.0 -- not a known variable star
05:56:52.45 +43:51:22.0 -- not a known variable star
05:56:58.08 +46:41:30.1 -- not a known variable star
05:57:12.05 +42:33:33.9 -- not a known variable star
05:57:28.83 +47:42:23.4 -- not a known variable star
05:57:30.26 +45:13:25.4 -- not a known variable star
05:57:40.02 +50:14:50.7 -- a known variable star
05:57:51.23 +50:11:53.6 -- not a known variable star
05:57:58.55 +48:05:37.9 -- not a known variable star
05:58:04.17 +45:09:36.8 -- not a known variable star
05:58:08.64 +46:59:24.3 -- not a known variable star
05:58:09.64 +48:37:13.4 -- not a known variable star
05:58:48.93 +42:14:42.8 -- not a known variable star
05:59:31.96 +48:16:11.9 -- not a known variable star
05:59:43.69 +47:14:06.7 -- not a known variable star
06:00:04.49 +45:58:33.7 -- not a known variable star
06:01:02.19 +47:22:16.2 -- not a known variable star
06:01:16.80 +47:35:46.1 -- not a known variable star
06:01:32.40 +47:32:26.8 -- not a known variable star
06:01:39.51 +45:44:14.4 -- not a known variable star
06:03:02.81 +46:44:00.0 -- a known variable star
06:03:15.22 +42:11:14.6 -- not a known variable star
06:03:40.60 +43:42:53.4 -- not a known variable star
06:04:44.11 +46:34:52.1 -- not a known variable star
06:04:49.69 +49:11:46.5 -- not a known variable star
06:05:14.75 +48:16:59.1 -- not a known variable star
06:05:45.84 +44:27:21.0 -- not a known variable star
06:07:09.27 +46:41:04.8 -- not a known variable star
06:07:50.11 +44:09:42.8 -- not a known variable star
06:08:02.31 +46:40:58.7 -- not a known variable star
06:08:37.44 +46:49:53.7 -- not a known variable star
06:08:52.42 +45:50:38.2 -- not a known variable star
06:09:09.96 +48:13:10.7 -- not a known variable star
06:09:37.13 +50:22:56.3 -- not a known variable star
06:10:00.20 +45:32:43.7 -- not a known variable star
06:10:20.57 +50:23:14.0 -- not a known variable star
06:10:50.08 +46:51:09.0 -- not a known variable star
06:12:43.11 +45:04:27.1 -- not a known variable star
06:13:09.37 +41:15:40.5 -- not a known variable star
06:13:29.81 +41:58:07.5 -- not a known variable star
06:13:33.63 +48:03:17.9 -- not a known variable star
06:15:16.65 +47:16:52.8 -- not a known variable star
06:18:00.66 +45:11:50.4 -- not a known variable star
06:18:02.57 +43:28:05.7 -- not a known variable star
06:20:59.78 +43:39:47.6 -- not a known variable star
06:21:48.17 +46:46:32.1 -- not a known variable star
06:24:00.40 +46:40:56.7 -- not a known variable star
06:25:47.82 +49:52:45.8 -- not a known variable star
06:25:48.93 +48:15:43.8 -- not a known variable star
06:26:19.88 +41:59:11.5 -- not a known variable star
06:26:29.80 +49:54:11.2 -- not a known variable star
06:28:33.70 +40:45:39.6 -- not a known variable star
06:38:26.78 +42:30:58.6 -- a known variable star
06:43:05.33 +46:46:43.5 -- not a known variable star
06:43:53.28 +49:12:00.2 -- not a known variable star
Found 136 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
158 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 158 (excluding asteroids and hot pixels, 136 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)2461140.70728206 -observatory V36
23:38:19.38 -04:54:17.4 Mercury (0.2mag)
02:40:36.07 +15:34:00.1 Venus (-3.9mag)
00:01:21.83 -00:57:00.2 Mars (1.2mag)
07:10:10.77 +22:50:10.1 Jupiter (-2.1mag)
00:26:34.89 +00:32:42.2 Saturn (0.9mag)
03:46:30.45 +19:43:38.7 Uranus (5.8mag)
00:10:04.35 -00:20:13.4 Neptune (7.8mag)
20:33:28.20 -22:52:27.0 Pluto (14.5mag)
19:31:57.05 -25:58:37.2 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Apr 10 00:49 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.70728206:
07:10:03.48 +22:50:23.3 Io (5.7mag)
07:10:18.13 +22:49:52.1 Europa (5.9mag)
07:10:08.88 +22:50:06.2 Ganymede (5.3mag)
07:09:49.50 +22:50:59.6 Callisto (6.6mag)
07:13:45.27 +22:40:35.8 Himalia (15.3mag)
07:10:07.20 +22:50:18.5 Thebe (16.2mag)
07:13:48.78 +23:10:08.0 Elara (17.3mag)
07:08:39.98 +23:33:12.2 Pasiphae (17.4mag)
07:18:37.88 +22:47:34.8 Carme (18.5mag)
00:26:44.86 +00:32:33.1 Titan (8.8mag)
00:26:33.59 +00:32:58.4 Rhea (10.1mag)
00:26:26.38 +00:33:44.9 Iapetus (11.5mag)
00:26:48.47 +00:32:31.0 Hyperion (14.8mag)
00:28:16.24 +00:42:07.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 10 00:49 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.70728206:
15:10:06.92 -11:50:45.0 JWST
19:23:19.37 +12:19:56.7 Chandra
08:02:52.28 -39:19:46.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 10 00:49 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.70728206 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:20.53 -28:27:00.2 13.9mag P/2010 H2 (Vales)
05:02:42.24 -69:56:36.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:16.43 +31:23:59.1 17.2mag C/2017 K2 (PANSTARRS)
17:30:51.24 +09:51:20.9 17.6mag C/2021 G2 (ATLAS)
23:08:35.67 +29:00:29.4 17.0mag C/2022 E2 (ATLAS)
04:22:32.72 +25:52:42.4 15.9mag C/2022 N2 (PANSTARRS)
09:02:21.51 +31:57:58.0 16.2mag C/2022 QE78 (ATLAS)
08:30:19.30 -00:46:48.9 17.3mag C/2022 R6 (PANSTARRS)
18:54:57.01 +18:02:27.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:26.48 -11:36:18.8 17.5mag P/2023 B1 (PANSTARRS)
09:10:32.07 -12:49:40.0 17.6mag C/2023 F3 (ATLAS)
21:48:06.15 +62:34:47.0 17.5mag C/2023 H5 (Lemmon)
19:23:46.66 -03:39:01.0 14.2mag C/2023 R1 (PANSTARRS)
21:40:33.07 +85:07:33.5 17.8mag C/2023 X2 (Lemmon)
06:15:35.31 +63:32:52.6 17.1mag C/2024 A1 (ATLAS)
05:00:28.74 +16:13:30.6 10.7mag C/2024 E1 (Wierzchos)
16:22:50.74 +05:26:18.9 17.4mag C/2024 G6 (ATLAS)
20:19:00.95 +13:43:29.8 14.7mag C/2024 J3 (ATLAS)
03:21:13.92 -23:16:55.3 16.4mag C/2024 T5 (ATLAS)
05:11:53.69 +46:45:51.2 17.7mag C/2025 J1 (Borisov)
14:02:52.20 +41:08:43.3 14.9mag C/2025 L1 (ATLAS)
03:16:18.94 -25:19:50.8 17.8mag C/2025 Q3 (ATLAS)
23:06:53.48 +19:42:29.4 9.4mag C/2025 R3 (PANSTARRS)
12:56:38.43 +02:39:07.7 17.5mag C/2025 Y1 (ATLAS)
02:30:24.84 +03:29:44.4 11.0mag C/2026 A1 (MAPS)
23:42:50.16 +36:05:54.3 14.4mag C/2026 B2 (Sun-Gao)
18:31:38.49 -10:01:19.1 12.2mag 10P/Tempel
15:07:58.26 +03:46:22.3 13.5mag 24P/Schaumasse
11:04:28.08 -01:43:13.4 15.7mag 29P/Schwassmann-Wachmann
17:58:50.22 -09:49:52.8 17.8mag 40P/Vaisala
10:38:06.26 -04:34:58.9 16.8mag 43P/Wolf-Harrington
01:39:43.51 +16:29:37.7 17.2mag 47P/Ashbrook-Jackson
07:00:16.89 +38:14:39.5 17.0mag 63P/Wild
23:21:35.44 -12:09:19.2 15.7mag 65P/Gunn
03:47:58.61 +19:12:56.2 15.9mag 76P/West-Kohoutek-Ikemura
00:52:49.67 +07:05:04.7 14.4mag 78P/Gehrels
22:45:12.95 -11:05:58.9 14.6mag 88P/Howell
01:54:10.61 +19:04:15.3 15.1mag 93P/Lovas
04:44:04.73 +31:57:59.6 16.3mag 123P/West-Hartley
08:21:53.45 +41:02:10.1 16.2mag 124P/Mrkos
02:24:18.79 +13:43:03.1 16.4mag 128P/Shoemaker-Holt
02:36:12.25 +13:46:20.6 17.5mag 131P/Mueller
00:56:06.94 +11:09:07.0 10.9mag 141P/Machholz
01:05:45.15 +02:41:50.4 11.0mag 141P-A/Machholz
23:54:01.61 -01:08:38.9 13.5mag 141P-D/Machholz
01:35:28.10 +04:25:06.3 17.9mag 141P-I/Machholz
00:46:15.66 -04:25:41.2 15.2mag 162P/SidingSpring
10:29:50.75 +31:14:59.9 17.9mag 164P/Christensen
06:25:48.08 +24:25:15.2 17.9mag 198P/ODAS
15:01:42.68 -00:42:20.3 17.5mag 210P/Christensen
21:21:35.16 -12:50:58.3 17.5mag 218P/LINEAR
17:14:37.17 -14:37:04.7 16.2mag 235P/LINEAR
05:22:04.90 +34:13:38.9 16.7mag 240P/NEAT
07:35:48.92 -05:48:48.3 17.7mag 242P/Spahr
15:44:44.03 +06:35:47.2 17.5mag 391P/Kowalski
07:32:07.68 +21:20:25.1 17.6mag 450P/LONEOS
05:27:31.81 +45:22:22.2 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 10 00:49 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 10 00:49 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
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
-rw-r--r-- 1 apache apache 187K Apr 10 00:49 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:24:18.822 -19:21:24.31 AT 2026ikf 2026-03-25.57 19.79
08:18:48.927 -23:32:12.08 AT 2026ike 2026-02-12.51 20.2
08:47:41.490 -21:46:40.10 AT 2026ikd 2026-03-28.41 19.49
08:34:30.248 -07:09:24.85 AT 2026ikc 2026-03-29.44 19.28
13:21:25.078 +79:09:18.53 AT 2026ikb 2026-03-25.43 20.7322
09:05:18.124 -19:48:21.41 AT 2026ika 2026-03-09.36 20.58
08:38:25.468 +06:11:03.79 AT 2026ijz 2026-03-09.32 21.99
08:00:34.010 +04:48:18.04 AT 2026ijy 2026-03-09.31 21.07
09:02:07.082 +07:27:03.87 AT 2026ijx 2026-02-17.43 21.29
10:37:20.784 +30:59:50.95 AT 2026ijw 2026-03-10.33 20.2
16:00:37.915 +06:38:30.61 AT 2026ijv 2026-03-28.57 20.5
13:51:30.137 +25:53:04.17 AT 2026iju 2026-03-28.41 20.07
12:52:01.341 -19:06:48.80 AT 2026ijt 2026-01-28.59 20.22
11:38:25.995 -11:34:40.48 AT 2026ijs 2026-01-16.56 21.1
07:12:41.661 +56:25:20.59 AT 2026ijr 2026-01-19.40 20.76
09:34:48.813 +06:57:40.76 AT 2026ijq 2026-01-26.43 21.57
10:49:59.384 +25:17:19.22 AT 2026ijp 2026-04-04.17 19.836
08:20:22.449 +03:44:22.06 AT 2026ijo 2026-04-02.18 19.8276
06:41:34.987 -19:08:36.17 AT 2026ijn 2026-02-05.26 20.38
12:35:13.975 +41:45:24.96 AT 2026ijm 2026-04-02.31 19.9925
-rw-r--r-- 1 apache apache 30K Apr 10 00:49 tns_transients_list.txt
