This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX
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 14.1372 2461144.6372 11.74 05:16:30.21 +45:55:23.3
162.63119 4.49691 galactic Aur Second-epoch detections are separated by 4.0" and 3.4 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 211733267699198720,2461144.6372,11.74,0.05,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
Large-amplitude variable Gaia DR2 211733267699198720 20260414.1372 11.74CV 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
AC Aur,2461144.6372,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Aur 20260414.1372 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055127.94+451129.9,2461144.6372,13.57,0.05,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
ASASSN-V J055127.94+451129.9 20260414.1372 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461144.6372,13.51,0.05,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
Gaia DR3 197994904265884544 20260414.1372 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,2461144.6372,13.41,0.05,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
target 20260414.1372 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,2461144.6372,13.34,0.05,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
target 20260414.1372 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
target,2461144.6372,13.52,0.05,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 20260414.1372 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211031122145549184,2461144.6372,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211031122145549184 20260414.1372 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
ATO J084.9379+44.9337,2461144.6372,13.16,0.05,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 J084.9379+44.9337 20260414.1372 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 J087.2715+41.2989,2461144.6372,12.94,0.05,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 J087.2715+41.2989 20260414.1372 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
ATO J090.6317+46.4867,2461144.6372,12.99,0.05,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 J090.6317+46.4867 20260414.1372 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
target,2461144.6372,13.12,0.05,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 20260414.1372 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060214.12+474700.6,2461144.6372,13.02,0.05,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
ASASSN-V J060214.12+474700.6 20260414.1372 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3673+41.8196,2461144.6372,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.3673+41.8196 20260414.1372 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192293833399060608,2461144.6372,12.66,0.05,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 192293833399060608 20260414.1372 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195531963862334720,2461144.6372,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195531963862334720 20260414.1372 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0152+49.4731,2461144.6372,12.72,0.05,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 J082.0152+49.4731 20260414.1372 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
target,2461144.6372,12.55,0.05,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 20260414.1372 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
ASASSN-V J062013.27+433839.0,2461144.6372,11.76,0.05,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
ASASSN-V J062013.27+433839.0 20260414.1372 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 J089.2879+46.2213,2461144.6372,11.01,0.05,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
ATO J089.2879+46.2213 20260414.1372 11.01CV 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
STARE aur0 543,2461144.6372,9.88,0.05,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
STARE aur0 543 20260414.1372 9.88CV 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 J084.3456+46.8139,2461144.6372,10.23,0.05,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
ATO J084.3456+46.8139 20260414.1372 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461144.6372,11.22,0.05,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
Gaia DR3 208934456550670592 20260414.1372 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963599002602153728,2461144.6372,11.67,0.05,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
Gaia DR3 963599002602153728 20260414.1372 11.67CV 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 J095.4408+46.7822,2461144.6372,11.93,0.05,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
ATO J095.4408+46.7822 20260414.1372 11.93CV 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
Gaia DR3 261967239550603520,2461144.6372,11.88,0.05,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
Gaia DR3 261967239550603520 20260414.1372 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 J085.0114+50.0334,2461144.6372,11.88,0.05,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
ATO J085.0114+50.0334 20260414.1372 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
Gaia DR3 197968717848571264,2461144.6372,12.07,0.05,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
Gaia DR3 197968717848571264 20260414.1372 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7984+46.2495,2461144.6372,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.7984+46.2495 20260414.1372 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.0101+43.3293,2461144.6372,12.12,0.05,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 J087.0101+43.3293 20260414.1372 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 194505775916838272,2461144.6372,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194505775916838272 20260414.1372 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,12.37,0.05,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
target 20260414.1372 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212655861031529216,2461144.6372,12.34,0.05,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 20260414.1372 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 214579559702388864,2461144.6372,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214579559702388864 20260414.1372 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053541.13+422836.6,2461144.6372,12.41,0.05,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
ASASSN-V J053541.13+422836.6 20260414.1372 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
ASASSN-V J054610.24+465447.5,2461144.6372,12.55,0.05,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
ASASSN-V J054610.24+465447.5 20260414.1372 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
target,2461144.6372,12.67,0.05,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
target 20260414.1372 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 J084.6086+42.9942,2461144.6372,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6086+42.9942 20260414.1372 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0489+43.4659,2461144.6372,12.60,0.05,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 J082.0489+43.4659 20260414.1372 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
ATO J082.7523+42.9146,2461144.6372,12.57,0.05,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
ATO J082.7523+42.9146 20260414.1372 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 J079.7145+41.1068,2461144.6372,12.47,0.05,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 J079.7145+41.1068 20260414.1372 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.9030+46.9269,2461144.6372,12.71,0.05,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 J091.9030+46.9269 20260414.1372 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
Gaia DR3 211485843219678720,2461144.6372,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211485843219678720 20260414.1372 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
Gaia DR3 967525667862574848,2461144.6372,12.78,0.05,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
Gaia DR3 967525667862574848 20260414.1372 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,12.62,0.05,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 20260414.1372 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,2461144.6372,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1372 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,12.74,0.05,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
target 20260414.1372 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207620613173739776,2461144.6372,12.64,0.05,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
Gaia DR3 207620613173739776 20260414.1372 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
target,2461144.6372,12.87,0.05,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 20260414.1372 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3627+42.0135,2461144.6372,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3627+42.0135 20260414.1372 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 192624786395334400,2461144.6372,12.74,0.05,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 192624786395334400 20260414.1372 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 J084.0658+43.5403,2461144.6372,12.75,0.05,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 J084.0658+43.5403 20260414.1372 12.75CV 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
Gaia DR3 968792687512124800,2461144.6372,12.99,0.05,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 968792687512124800 20260414.1372 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
target,2461144.6372,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1372 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3774+41.9686,2461144.6372,12.96,0.05,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 J093.3774+41.9686 20260414.1372 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8834+47.5321,2461144.6372,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8834+47.5321 20260414.1372 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
target,2461144.6372,13.10,0.05,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 20260414.1372 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,2461144.6372,12.98,0.05,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 20260414.1372 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461144.6372,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3195+44.0466 20260414.1372 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,12.91,0.05,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
target 20260414.1372 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461144.6372,13.03,0.05,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
Gaia DR3 197388553666998656 20260414.1372 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 J090.6351+48.1884,2461144.6372,12.96,0.05,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 J090.6351+48.1884 20260414.1372 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,2461144.6372,12.99,0.05,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
target 20260414.1372 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 J095.7693+49.1987,2461144.6372,13.07,0.05,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
ATO J095.7693+49.1987 20260414.1372 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3023+47.5982,2461144.6372,12.99,0.05,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 J090.3023+47.5982 20260414.1372 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
target,2461144.6372,13.03,0.05,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
target 20260414.1372 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 214264171664738816,2461144.6372,13.06,0.05,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
Gaia DR3 214264171664738816 20260414.1372 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,2461144.6372,13.12,0.05,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 20260414.1372 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 211466700549060736,2461144.6372,13.12,0.05,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
Gaia DR3 211466700549060736 20260414.1372 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1559+40.9633,2461144.6372,13.21,0.05,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
ATO J090.1559+40.9633 20260414.1372 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197673090956515200,2461144.6372,13.16,0.05,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 197673090956515200 20260414.1372 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,13.07,0.05,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 20260414.1372 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962460256449852032,2461144.6372,13.20,0.05,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
Gaia DR3 962460256449852032 20260414.1372 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
ATO J084.7593+47.5882,2461144.6372,13.12,0.05,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 J084.7593+47.5882 20260414.1372 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 963318524057490944,2461144.6372,13.37,0.05,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 963318524057490944 20260414.1372 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5567+44.2856,2461144.6372,13.18,0.05,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 J083.5567+44.2856 20260414.1372 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
Gaia DR3 213847422398656512,2461144.6372,13.27,0.05,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
Gaia DR3 213847422398656512 20260414.1372 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
target,2461144.6372,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260414.1372 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 197666322088101120,2461144.6372,13.22,0.05,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
Gaia DR3 197666322088101120 20260414.1372 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
target,2461144.6372,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1372 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461144.6372,13.21,0.05,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
ATO J083.5805+44.4532 20260414.1372 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 J089.2887+47.4652,2461144.6372,13.40,0.05,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 J089.2887+47.4652 20260414.1372 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 961873220320094848,2461144.6372,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 961873220320094848 20260414.1372 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461144.6372,13.23,0.05,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
ATO J084.1629+50.0440 20260414.1372 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 J092.6873+48.2843,2461144.6372,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.6873+48.2843 20260414.1372 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.6698+46.3547,2461144.6372,13.40,0.05,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 J087.6698+46.3547 20260414.1372 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
target,2461144.6372,13.51,0.05,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 20260414.1372 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,2461144.6372,13.56,0.05,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 20260414.1372 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,2461144.6372,13.70,0.05,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 20260414.1372 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,13.62,0.05,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 20260414.1372 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 970794206694859904,2461144.6372,13.63,0.05,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
Gaia DR3 970794206694859904 20260414.1372 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,13.78,0.05,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 20260414.1372 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 198142646844130816,2461144.6372,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 198142646844130816 20260414.1372 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3650+48.6832,2461144.6372,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.3650+48.6832 20260414.1372 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197048602713243776,2461144.6372,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197048602713243776 20260414.1372 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 965274903137379968,2461144.6372,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 965274903137379968 20260414.1372 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6372,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1372 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1772+47.3666,2461144.6372,13.88,0.05,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
ATO J089.1772+47.3666 20260414.1372 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
VY Aur,2461144.6372,11.51,0.05,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
VY Aur 20260414.1372 11.51CV 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
## 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: 2461144.63755336 14.04.2026 03:17:54.610 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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: 8 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): 22990
Objects passed selection criteria: 22964
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: 20395.5
Average stars matched: 19954.8 (97.839 %)
Memory usage VmPeak: 126876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:21:09 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: 2461144.63755336 14.04.2026 03:17:54.610 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 363
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: 133 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): 161332
Objects passed selection criteria: 161000
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 149734
Average stars matched: 145280 (97.0251 %)
Memory usage VmPeak: 1982080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:25:36 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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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: 2461144.63689470
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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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 06:00:19.752 +45:59:58.72
Angular distance between the image centers 0.0930 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 06:00:21.502 +46:00:06.79
Angular distance between the image centers 0.0978 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 06:00:19.752 +45:59:58.72
Second-epoch second image center 06:00:21.502 +46:00:06.79
Angular distance between the image centers 0.00554 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.wecy03egUA
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.Mkxg1MvVkH
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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits &> /tmp/tmp.m0xO0pbBb8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits &> /tmp/tmp.g0d7Ia8BVU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
15.0 mag. fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wecy03egUA (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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.Mkxg1MvVkH (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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.m0xO0pbBb8 (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1142, passed=16832
Got 16832 stars (including 15671 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat
util/solve_plate_with_UCAC5 got 16832 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 16440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 16440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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.g0d7Ia8BVU (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1096, passed=16686
Got 16686 stars (including 15569 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat
util/solve_plate_with_UCAC5 got 16686 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 16348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 927 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(), 16349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 16349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 925 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31636.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 2s
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Considering the candidate 31504_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31504_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:46.15 +43:34:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31548_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31548_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:34:27.46 +44:52:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 1.266 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31555_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31555_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:14:59.12 +46:47:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31569_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31569_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:59:43.43 +44:59:09.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31573_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31573_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:28.52 +43:00:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31574_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31574_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:23.08 +46:49:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.670 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31581_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31581_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:27:42.21 +43:22:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31636_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 31636_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 31647_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31647_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31673_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31673_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:21.22 +50:18:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31702_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31702_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:28:45.83 +48:34:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.487 967547868550025216 097.19110438442 +48.57701626020 12.2587 11.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31703_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 31703_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:26:31.29 +42:40:34.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:26:01.83 +50:29:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:41:12.82 +44:09:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 20s
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 ####
05:27:04.81 +50:07:23.9
05:16:30.21 +45:55:23.3
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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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 06:00:19.752 +45:59:58.72
Angular distance between the image centers 0.0930 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 06:00:21.502 +46:00:06.79
Angular distance between the image centers 0.0978 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 06:00:19.752 +45:59:58.72
Second-epoch second image center 06:00:21.502 +46:00:06.79
Angular distance between the image centers 0.00554 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.i7QxeAQV9T
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.6ybsYb3XYj
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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits &> /tmp/tmp.y9mlwEYKsd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits &> /tmp/tmp.8P9CE7cnVW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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 350 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
2.1 pix fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
2.1 pix fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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
14.0 mag. fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
14.0 mag. fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.i7QxeAQV9T (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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.6ybsYb3XYj (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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.y9mlwEYKsd (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=10745, passed=131831
Got 131831 stars (including 120854 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat
util/solve_plate_with_UCAC5 got 131831 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 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(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 129462 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 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 129464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 129464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 933 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_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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.8P9CE7cnVW (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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=10279, passed=129606
Got 129606 stars (including 119115 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat
util/solve_plate_with_UCAC5 got 129606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 127065 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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 127064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 127066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/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_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-16-57_20.00sec_-4.90C_LIGHTs_0061.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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_2026-04-13_CI_Aur-02-Q1b1x1_221846_TTUQ1b1x1_16025_2got0hPX/wcs_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062.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__out195208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out195235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68332.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 135s
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: 62s
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Considering the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195205_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:45:48.57 +50:04:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.931 214179440549445376 086.45312218175 +50.07090692024 14.4019 13.3260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195208_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195208_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:04:12.79 +50:13:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.091 970415910271615232 091.05354351434 +50.22491000811 14.7079 14.1289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195220_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195220_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:06:24.42 +44:04:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.333 961235263057938432 091.60190927977 +44.06746322477 14.7221 14.1584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195221_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195221_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:25:36.44 +48:19:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195222_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195222_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:54:36.09 +50:36:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.551 211624759642265728 088.65051018604 +50.61021009047 14.6311 14.0005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195226_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195226_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:34:16.28 +46:57:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195231_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195231_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:36.75 +47:42:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.865 969703667255081728 090.90347088593 +47.71592073831 14.4357 13.8490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195235_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195235_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195252_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195252_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:14.79 +48:35:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.310 210418389227972480 089.06258872810 +48.59656553123 14.3443 13.5711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195257_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195257_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195259_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195259_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:36:15.68 +49:01:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195261_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195261_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:30.77 +44:43:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195262_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195262_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:54:04.12 +50:05:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.803 211551161082978432 088.51749029006 +50.09856694290 14.2592 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195264_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195264_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:41:26.76 +43:07:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195266_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195266_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:50:32.86 +42:15:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195276_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195276_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:48:03.44 +49:48:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195278_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195278_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195282_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195282_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:05:45.75 +44:27:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.316 962934901876874880 091.44102792761 +44.45555912510 14.1989 13.6480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195284_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195284_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195288_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195288_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:15:40.13 +41:53:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195298_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195298_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195310_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195310_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:10:34.44 +50:01:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195312_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195312_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195313_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:44:36.84 +46:43:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.295 209668384859666048 086.15384962110 +46.72668476459 13.9845 13.4608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195315_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:09.12 +45:22:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.899 196739021469243136 089.28834194525 +45.38023735729 13.9714 13.3170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195318_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195318_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:52:59.21 +46:57:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195322_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195322_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195325_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195325_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:21:49.28 +47:17:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.870 211950180726200960 080.45553127216 +47.28875661514 13.9802 13.3201 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 195326_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195326_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:06.64 +50:40:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195328_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195328_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:25:37.68 +42:12:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195333_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:26:15.95 +44:02:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195336_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195336_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:25.95 +49:51:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195337_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195337_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195339_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195339_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:34:05.55 +48:22:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195340_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195340_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:43.66 +50:23:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195342_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195342_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:17:08.74 +49:40:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195343_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195343_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:25:18.44 +47:51:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195344_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195344_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:53.98 +47:59:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195347_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195347_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:53:03.28 +44:04:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.169 196514136982442624 088.26444235659 +44.07375640630 13.5476 12.8497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195349_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:59.20 +46:26:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.988 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195350_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:36:57.63 +44:14:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195351_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195351_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195352_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195352_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195355_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195355_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:31:27.62 +47:36:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195356_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195356_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195364_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:47.31 +41:40:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195365_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195365_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:32:53.65 +50:04:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195369_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195369_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195371_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195371_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:16:36.18 +44:32:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.901 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195372_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195372_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:32:56.95 +44:10:53.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195376_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:16:43.86 +44:42:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.129 962379987803965824 094.18319043390 +44.71153534768 13.5579 13.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195377_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:19:47.30 +42:06:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195379_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195379_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:51:22.30 +51:05:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195380_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195380_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:30:25.32 +44:55:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195382_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:21:00.04 +43:23:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195384_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195384_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:01.71 +46:28:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.694 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195388_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:22:39.62 +47:54:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.692 212586660519063680 080.66597215012 +47.91400751652 13.0455 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195391_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195391_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:26:51.33 +41:14:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 1.483 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195392_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195392_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:24.06 +41:20:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195401_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:23.54 +49:53:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195402_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195402_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:32:37.14 +41:20:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195403_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195403_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:25:35.50 +49:58:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195404_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195404_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 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 195405_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195405_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:03.08 +42:12:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195407_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195407_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:00:34.55 +45:32:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.699 963062342146066432 090.14422902412 +45.53343101528 12.7393 12.0346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195408_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195408_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195411_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:54:42.14 +43:39:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.349 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195412_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:45.95 +43:34:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195413_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195413_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195416_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195416_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:28:39.58 +41:12:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195470_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195470_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195483_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:43:27.54 +42:19:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.12, MAG_FAINT_SEARCH_LIMIT=11.10)GAIADR2_OUTPUT=# 0.196 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195484_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195484_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:28.51 +43:00:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195501_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195501_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195543_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195543_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195563_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195593_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195593_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:11:34.52 +48:44:35.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195602_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195602_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 195608_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195608_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 195622_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195622_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195648_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195648_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 195658_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195658_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:43:31.81 +50:41:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.383 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195676_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195676_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:46:26.54 +47:55:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.023 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195679_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195679_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:19:01.51 +41:06:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195685_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195685_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 195686_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195686_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:19:04.18 +47:21:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.755 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195689_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195689_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:23.66 +44:31:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195693_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195693_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 195694_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195694_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:06:21.34 +48:46:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.507 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195699_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195699_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195709_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195709_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:36:59.24 +48:07:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.276 967332673508208256 099.24717563820 +48.11763216666 12.6763 12.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195715_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195715_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 195761_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195761_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:13:46.62 +44:43:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.510 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195764_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195764_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 195765_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195765_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195771_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195771_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195776_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195776_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195777_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195777_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:18:23.56 +48:55:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195779_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195779_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:32:51.83 +42:57:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195791_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195791_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:07.54 +44:53:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.278 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195797_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195797_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:48.29 +46:57:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.995 198029362786762880 089.20161100133 +46.96494369065 12.8922 12.0517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195798_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195798_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:05:50.16 +44:39:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.906 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195809_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195809_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195810_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195810_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 195825_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195825_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195827_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195827_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:07.67 +50:04:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.577 214356977317827200 085.53219554945 +50.07566096651 13.0436 12.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195838_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195838_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:17:56.60 +46:08:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195843_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195843_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:40.86 +44:01:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.977 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195859_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195859_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195878_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195878_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:11.06 +43:58:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195884_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195884_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:15.24 +49:29:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.719 970317499685347200 090.81417500874 +49.49589386941 13.2117 12.4205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195887_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195887_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:12:10.12 +50:14:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195888_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195888_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:46.06 +45:53:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.042 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:13.58 +42:56:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195894_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195894_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195898_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195898_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:25.83 +48:47:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195899_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195899_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:53.87 +49:47:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195901_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:42.95 +48:20:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.176 210971336200363648 085.17944784055 +48.33622155749 13.2097 12.6468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195911_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195911_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:17:28.74 +45:52:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.678 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195913_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195913_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:02.39 +49:49:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.895 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195916_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195916_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:47:58.48 +50:54:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195924_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195924_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195927_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195927_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195932_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195932_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:11:06.01 +41:55:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.055 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195942_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 195942_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 195957_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195957_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:11:01.05 +47:29:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.118 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195959_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195959_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:32.58 +43:42:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.630 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195965_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195965_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:29:04.66 +42:17:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195967_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195967_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:59:52.71 +44:00:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.451 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195982_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195982_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:47:45.26 +50:03:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.352 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195988_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195988_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:17:34.73 +46:23:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195993_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195993_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:40.69 +41:28:15.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195996_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195996_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:17:15.75 +41:56:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.467 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 195997_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:35:17.67 +42:18:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196006_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:53:12.05 +45:24:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.357 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196010_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196010_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196035_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196035_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:33:56.50 +46:11:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.350 208282721033602560 083.48553101272 +46.19874907056 13.4787 12.6535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196042_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196042_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196044_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196044_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:44.71 +49:06:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196046_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196046_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:13:42.35 +45:31:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196054_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196054_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:55:48.03 +42:30:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196058_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196058_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:52.04 +41:16:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.237 194180797215485440 081.21738962468 +41.28187659990 12.4521 11.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196061_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196061_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:53:17.94 +43:17:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196073_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196073_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196079_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196079_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:59.24 +46:40:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196081_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196081_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:22.98 +42:40:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196082_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196082_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:44.77 +44:40:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.635 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196089_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196089_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:57.15 +43:05:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196094_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196094_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196102_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196102_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:41.15 +48:21:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196107_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196107_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:09.32 +46:12:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.698 209019462542689408 082.53951456145 +46.21579217952 13.5370 12.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196111_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196111_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:43:06.41 +44:51:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.707 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196115_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196115_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:14.25 +50:00:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196118_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196118_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:22:53.74 +48:33:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196120_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196120_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196123_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196123_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196128_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196128_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196136_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196136_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:22:05.63 +48:44:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196138_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196138_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196140_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196140_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196151_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196151_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:52:03.69 +49:32:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196154_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196154_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:44:48.13 +48:58:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196155_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196155_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:12:03.03 +41:43:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.484 960200034204636544 093.01317175941 +41.73174612260 13.5765 12.8505 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#
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Considering the candidate 196157_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196157_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196159_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196159_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:21:51.04 +46:21:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196163_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196163_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196166_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:23:51.23 +41:27:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.397 194936475237258624 080.96419664108 +41.46092571425 13.5029 12.4255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196169_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196169_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:46.46 +46:04:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.248 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196171_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196171_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:16:35.87 +45:44:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196180_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196180_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:27:03.62 +46:04:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196183_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196183_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:27:28.21 +42:15:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196188_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196188_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:22:02.11 +42:43:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.008 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196192_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196192_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196194_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196194_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 196195_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196195_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:02:48.81 +43:13:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196200_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196200_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:31:01.91 +44:18:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196201_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196201_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:22.04 +42:59:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.024 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196202_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196202_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:31:40.24 +42:51:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196207_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196207_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:02:52.40 +45:42:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.778 963146592224643200 090.71840891408 +45.70231821898 13.6956 12.9106 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 196209_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196212_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196212_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:00:14.00 +47:43:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.161 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196214_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196214_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:25:57.48 +43:06:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.715 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196217_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196217_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:26:13.33 +46:47:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196227_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196227_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:46:39.71 +43:21:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196228_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196228_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:32.56 +41:57:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196233_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196233_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196235_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196235_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:22:30.73 +46:12:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.332 968436170866744448 095.62879686623 +46.20538276046 13.7294 12.9970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196242_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196242_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196256_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196256_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196261_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196261_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:28.18 +42:14:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196262_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196262_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:32:30.31 +41:38:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196268_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196268_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:53:08.59 +50:16:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196278_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196278_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:24.80 +44:48:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.227 208086290707268608 081.10372106703 +44.80994290569 13.9169 13.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196279_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196279_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:28:50.43 +44:16:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196284_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196284_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:50.69 +48:07:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.209 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196286_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196286_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196287_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196287_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196296_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196296_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:18:58.08 +43:42:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.100 207515987770326784 079.74275755653 +43.70229955072 13.6619 12.7892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196297_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196297_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:52:47.02 +41:21:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196298_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196298_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:06.21 +45:12:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196301_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196301_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:25:45.38 +45:22:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196311_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196311_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:27.83 +47:51:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196319_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196319_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:24:21.74 +47:52:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196327_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196327_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:38:50.47 +49:49:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196339_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196339_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:20:27.54 +46:35:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196351_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196351_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196352_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:26:28.18 +42:41:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196353_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196353_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:59:59.07 +43:51:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196354_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196354_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196355_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196355_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:31:17.62 +46:25:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196357_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196357_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196358_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196358_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:47:49.19 +51:04:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196373_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196373_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:33.67 +45:29:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196374_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196374_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196377_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196377_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196379_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196379_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196383_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196383_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196386_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196386_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:02:54.83 +43:29:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.440 961296354673535104 090.72898800763 +43.48533345261 13.7915 13.0128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196394_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196394_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:33:32.15 +48:16:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.738 212436955138189696 083.38339755979 +48.28147147774 13.9515 13.4567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196399_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196399_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196415_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196415_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:18:32.68 +46:16:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.389 211837721303196800 079.63671201134 +46.28305578216 13.5567 13.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196422_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196422_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:15:49.31 +47:42:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.363 968813234635537152 093.95590182109 +47.71357261547 13.8786 13.1179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196426_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196426_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:08:18.97 +41:46:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196429_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196429_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:20:02.68 +46:37:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196435_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196435_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:19:18.31 +46:15:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196442_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196442_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:24.75 +49:14:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196445_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196445_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:23:54.16 +46:06:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196450_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196450_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196451_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196451_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:43:56.56 +47:43:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.529 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196452_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196452_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:13:33.57 +48:03:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.529 969210708089081216 093.39001337563 +48.05522019758 14.0114 13.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196455_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196455_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:47:28.62 +41:25:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196457_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196457_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196461_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196461_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:18.13 +49:09:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.985 212754370401019392 082.57660163312 +49.15706591744 13.9463 13.3591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196488_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196488_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:28:18.28 +44:16:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.683 207789005953568000 082.07681950966 +44.26697163248 13.7769 12.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196497_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196497_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:39.47 +41:06:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196503_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196503_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:51:56.95 +41:37:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.563 192277649962098688 087.98771623166 +41.62337032686 13.8897 13.1157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196509_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196509_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196510_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196510_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:28:45.58 +49:11:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196518_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196518_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:48:44.69 +49:34:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.454 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196523_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196523_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196529_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196529_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:19:50.38 +45:03:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.852 208529600051866240 079.96005250816 +45.06203311659 13.7148 12.6649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196539_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196539_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:55:48.22 +42:30:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196543_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196543_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196554_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196554_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:34.10 +46:53:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196559_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:25:04.93 +42:33:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196565_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196565_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196573_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196573_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 196576_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196576_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196578_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196578_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:23:09.74 +49:09:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.030 970593653198168064 095.79099454777 +49.16629137386 14.1385 13.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196580_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196580_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:12:20.08 +50:12:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.472 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196581_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196581_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:22:08.12 +41:29:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196600_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196600_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:11:51.64 +45:03:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.935 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196603_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196603_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:36:18.59 +47:12:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.855 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196610_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196610_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 196619_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196619_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:55:50.47 +42:45:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196621_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196621_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:36:57.49 +42:25:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196623_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196623_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:52:21.04 +42:50:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196628_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196628_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:21.20 +42:41:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196630_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196630_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:00.76 +49:05:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.448 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196633_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196633_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:11.30 +42:50:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.439 192511364902195840 089.29695470380 +42.84027162771 14.0339 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196640_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196640_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196641_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196641_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196642_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196642_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:15.61 +45:20:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196648_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196648_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:43.63 +50:12:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196651_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196651_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196656_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196656_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:34:00.78 +46:20:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.641 208287501334038656 083.50390290064 +46.33909529807 14.0153 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196662_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196662_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196670_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196670_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196678_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196678_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:35:41.25 +44:16:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196687_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196687_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196690_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196690_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:50:06.44 +46:08:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196698_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196698_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:01:09.36 +43:25:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.084 961328240510820608 090.28939859901 +43.42708214892 14.1712 13.3742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196700_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196700_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196716_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196716_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:53.20 +46:05:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.525 197005378160950784 089.47179707530 +46.09439219961 14.0011 13.1854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196723_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196723_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:26:12.67 +49:06:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.141 970669347702108288 096.55228667167 +49.11057778149 13.8025 12.7263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196729_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196729_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196731_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196731_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 196746_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196746_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196749_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196749_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196756_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196756_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:41:07.37 +47:58:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196760_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196760_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196764_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196764_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:42:47.33 +45:58:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196771_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196771_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:04:15.37 +46:54:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.876 963649000318538496 091.06438493489 +46.91042639042 14.3324 13.7065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196782_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196782_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:44.61 +42:36:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.808 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196783_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196783_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196786_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196786_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:49:38.71 +47:49:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.599 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196795_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196795_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:16.97 +47:02:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196809_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196809_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196850_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196850_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:10:13.55 +49:41:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.795 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196853_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196853_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:23.52 +49:49:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196855_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196855_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196865_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:13.61 +44:55:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196872_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196872_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:33.86 +49:48:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.271 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:22:50.26 +48:57:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196911_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196911_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 196913_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196913_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196915_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196915_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:26:12.84 +50:13:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.209 971125473228480896 096.55402464209 +50.21828138308 14.3857 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196917_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196917_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:40:28.06 +46:16:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196919_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196919_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:03:02.76 +46:43:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.455 963597151473005312 090.76167548963 +46.73289191284 14.4883 13.8730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196930_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196930_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:09:37.23 +50:22:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.002 971732094409236096 092.40552932955 +50.38177186496 14.5645 13.9943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196939_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196939_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 196941_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196941_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196960_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196960_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:54:21.45 +42:55:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.058 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196967_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196967_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:31:34.92 +50:10:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.890 213632021198277376 082.89588145654 +50.18223210576 14.3987 13.5553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196978_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 196978_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 196985_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 196985_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:25:22.21 +44:07:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.557 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197013_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197013_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197014_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197014_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:10:00.28 +45:32:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.781 963235820168851712 092.50109436752 +45.54496087176 14.4482 13.9808 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#
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Considering the candidate 197029_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197029_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197040_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197040_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197048_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197048_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197052_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197052_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197055_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197055_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197059_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197059_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
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Considering the candidate 197073_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197073_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:43:51.85 +48:54:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.603 967062709043660672 100.96671507987 +48.90653583707 14.8000 14.2973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197091_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197091_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:30:47.06 +47:20:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.651 209357978983188864 082.69669623066 +47.34752735043 14.4460 13.8493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197105_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197105_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:04:02.02 +42:01:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197111_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197111_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:01:32.45 +48:06:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.788 969772008774566528 090.38550220391 +48.10359754765 14.5671 13.9081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197112_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197112_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:13:34.86 +47:17:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.081 968786021723106432 093.39565799104 +47.29035592636 14.7016 14.0192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197117_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197117_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:56:15.11 +43:27:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.852 193317989823389312 089.06301907741 +43.46567683731 14.9508 14.3701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197134_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197134_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:39:18.68 +46:40:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.926 209759575604369920 084.82861277952 +46.67351168016 14.8166 14.1638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197159_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197159_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:14.19 +46:00:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.183 209520122588849024 084.30995072691 +46.00355328020 14.7209 14.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197166_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197166_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:10:00.28 +46:40:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.758 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197169_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197169_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197214_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197214_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:59:51.36 +51:05:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.540 211664376420455168 089.96466731365 +51.09810907484 14.6737 14.0602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197236_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197236_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:00:13.82 +47:42:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.015 963734826647553152 090.05830054204 +47.71388332991 14.8111 14.1290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197238_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197238_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:44:51.20 +50:14:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.925 214198407124868608 086.21406793502 +50.24292183154 14.7953 14.1920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197254_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 197254_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197288_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197288_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:10.39 +47:17:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.433 210624925615467392 084.29384731994 +47.29912810693 14.6770 14.0165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197290_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197290_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:02:02.53 +41:50:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.393 960759896078081536 090.51141856402 +41.84365110628 14.7475 14.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197301_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 197301_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:34:08.53 +44:17:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.171 195826594321239040 083.53574128686 +44.28348556654 14.4393 13.6154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 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 102378_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:37:56.95 +44:41:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:57:23.98 +48:22:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:27:04.82 +50:07:23.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:21:29.80 +43:44:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 05:59:44.08 +47:37:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-13_22-17-54_20.00sec_-4.90C_LIGHTs_0062 did not pass the final checks
**** FOUND 06:26:01.80 +50:29:26.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 203s
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 ####
05:27:04.81 +50:07:23.9
05:16:30.21 +45:55:23.3
05:51:27.82 +45:11:28.1
05:53:04.76 +46:58:02.0
05:42:47.66 +50:22:59.9
06:35:26.95 +44:24:50.4
06:14:03.05 +50:52:47.6
05:46:41.19 +49:10:47.8
05:39:45.66 +44:56:08.8
05:49:04.53 +41:17:27.2
06:02:31.73 +46:29:05.9
06:04:53.14 +50:08:48.5
06:02:14.09 +47:47:00.1
06:21:31.91 +41:49:30.9
05:54:06.60 +41:46:10.4
05:36:11.28 +43:24:36.5
05:28:04.10 +49:28:29.9
05:38:27.37 +41:13:50.9
06:20:12.78 +43:38:52.8
05:57:09.01 +46:13:43.3
05:17:54.81 +41:11:55.2
05:37:22.99 +46:49:18.2
05:25:37.69 +45:40:56.6
06:02:11.23 +46:42:58.2
06:21:48.08 +46:46:31.6
05:29:21.92 +51:11:33.0
05:40:02.91 +50:02:04.5
05:48:45.93 +46:35:01.2
05:51:18.29 +46:14:40.9
05:48:04.06 +43:19:50.4
05:28:43.85 +41:18:08.9
06:26:19.86 +41:59:11.1
05:28:01.23 +48:14:57.8
05:48:00.92 +50:37:40.6
05:35:42.14 +42:29:13.7
05:46:10.04 +46:54:48.0
05:51:03.49 +47:53:56.1
05:38:24.31 +42:59:48.0
05:28:11.70 +43:27:56.1
05:31:00.44 +42:54:52.6
05:18:50.14 +41:06:32.4
06:07:29.96 +46:55:56.8
05:48:23.18 +49:46:57.8
06:25:48.90 +48:15:43.2
05:27:26.03 +44:48:51.3
05:27:50.99 +42:20:24.9
05:22:47.43 +47:00:53.7
05:20:50.90 +44:04:36.6
05:57:45.30 +45:54:52.2
05:37:28.33 +42:00:46.1
05:40:57.34 +41:07:45.3
05:36:14.40 +43:32:31.4
06:12:44.88 +47:30:43.0
05:44:39.75 +43:57:55.6
06:13:29.68 +41:58:06.6
05:35:36.13 +47:32:42.0
06:40:19.79 +44:20:22.7
05:53:51.64 +50:42:48.8
05:37:16.23 +44:02:46.1
05:51:18.88 +43:17:46.0
05:37:19.32 +44:51:38.1
06:02:32.03 +48:11:24.7
06:00:04.54 +45:58:32.6
06:23:05.38 +49:11:45.9
06:01:16.78 +47:35:44.8
05:42:16.22 +43:16:25.6
05:38:36.16 +49:43:22.4
06:26:29.81 +49:54:10.2
05:48:07.92 +49:40:41.4
06:00:41.16 +40:57:37.0
05:49:15.53 +45:41:16.2
05:57:12.02 +42:33:32.7
06:13:27.72 +45:03:37.2
05:38:59.89 +47:35:32.0
06:07:54.28 +45:58:48.7
05:34:15.83 +44:17:05.5
05:31:08.96 +50:39:12.8
05:37:52.47 +43:02:34.3
05:48:10.11 +45:27:38.2
05:59:26.46 +46:32:41.8
05:34:18.90 +44:27:44.5
05:57:12.02 +47:27:16.4
06:14:21.48 +43:11:50.6
05:36:40.83 +50:02:55.4
06:10:45.05 +48:16:57.3
05:50:43.76 +46:21:03.3
06:05:19.87 +49:43:46.5
06:25:47.98 +49:52:45.3
06:38:58.52 +48:06:11.7
05:56:05.19 +44:35:31.1
06:20:46.17 +50:02:59.8
06:41:34.47 +49:47:47.0
05:57:28.48 +47:42:20.7
05:33:27.71 +48:41:06.2
05:39:25.73 +43:54:06.0
06:25:16.30 +45:04:14.5
06:06:36.45 +47:00:44.4
05:56:44.19 +47:22:14.9
06:09:51.91 +46:34:27.7
########### 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 ####
05:16:30.21 +45:55:23.3
05:27:04.81 +50:07:23.9
05:51:27.82 +45:11:28.1
05:53:04.76 +46:58:02.0
05:42:47.66 +50:22:59.9
06:35:26.95 +44:24:50.4
06:14:03.05 +50:52:47.6
05:46:41.19 +49:10:47.8
05:39:45.66 +44:56:08.8
05:49:04.53 +41:17:27.2
06:02:31.73 +46:29:05.9
06:04:53.14 +50:08:48.5
06:02:14.09 +47:47:00.1
06:21:31.91 +41:49:30.9
05:54:06.60 +41:46:10.4
05:36:11.28 +43:24:36.5
05:28:04.10 +49:28:29.9
05:38:27.37 +41:13:50.9
06:20:12.78 +43:38:52.8
05:57:09.01 +46:13:43.3
05:17:54.81 +41:11:55.2
05:37:22.99 +46:49:18.2
05:25:37.69 +45:40:56.6
06:02:11.23 +46:42:58.2
06:21:48.08 +46:46:31.6
05:29:21.92 +51:11:33.0
05:40:02.91 +50:02:04.5
05:48:45.93 +46:35:01.2
05:51:18.29 +46:14:40.9
05:48:04.06 +43:19:50.4
05:28:43.85 +41:18:08.9
06:26:19.86 +41:59:11.1
05:28:01.23 +48:14:57.8
05:48:00.92 +50:37:40.6
05:35:42.14 +42:29:13.7
05:46:10.04 +46:54:48.0
05:51:03.49 +47:53:56.1
05:38:24.31 +42:59:48.0
05:28:11.70 +43:27:56.1
05:31:00.44 +42:54:52.6
05:18:50.14 +41:06:32.4
06:07:29.96 +46:55:56.8
05:48:23.18 +49:46:57.8
06:25:48.90 +48:15:43.2
05:27:26.03 +44:48:51.3
05:27:50.99 +42:20:24.9
05:22:47.43 +47:00:53.7
05:20:50.90 +44:04:36.6
05:57:45.30 +45:54:52.2
05:37:28.33 +42:00:46.1
05:40:57.34 +41:07:45.3
05:36:14.40 +43:32:31.4
06:12:44.88 +47:30:43.0
05:44:39.75 +43:57:55.6
06:13:29.68 +41:58:06.6
05:35:36.13 +47:32:42.0
06:40:19.79 +44:20:22.7
05:53:51.64 +50:42:48.8
05:37:16.23 +44:02:46.1
05:51:18.88 +43:17:46.0
05:37:19.32 +44:51:38.1
06:02:32.03 +48:11:24.7
06:00:04.54 +45:58:32.6
06:23:05.38 +49:11:45.9
06:01:16.78 +47:35:44.8
05:42:16.22 +43:16:25.6
05:38:36.16 +49:43:22.4
06:26:29.81 +49:54:10.2
05:48:07.92 +49:40:41.4
06:00:41.16 +40:57:37.0
05:49:15.53 +45:41:16.2
05:57:12.02 +42:33:32.7
06:13:27.72 +45:03:37.2
05:38:59.89 +47:35:32.0
06:07:54.28 +45:58:48.7
05:34:15.83 +44:17:05.5
05:31:08.96 +50:39:12.8
05:37:52.47 +43:02:34.3
05:48:10.11 +45:27:38.2
05:59:26.46 +46:32:41.8
05:34:18.90 +44:27:44.5
05:57:12.02 +47:27:16.4
06:14:21.48 +43:11:50.6
05:36:40.83 +50:02:55.4
06:10:45.05 +48:16:57.3
05:50:43.76 +46:21:03.3
06:05:19.87 +49:43:46.5
06:25:47.98 +49:52:45.3
06:38:58.52 +48:06:11.7
05:56:05.19 +44:35:31.1
06:20:46.17 +50:02:59.8
06:41:34.47 +49:47:47.0
05:57:28.48 +47:42:20.7
05:33:27.71 +48:41:06.2
05:39:25.73 +43:54:06.0
06:25:16.30 +45:04:14.5
06:06:36.45 +47:00:44.4
05:56:44.19 +47:22:14.9
06:09:51.91 +46:34:27.7
###################################################################################
05:16:30.21 +45:55:23.3 -- not an asteroid (will add it to exclusion list)
05:27:04.81 +50:07:23.9 -- not an asteroid (will add it to exclusion list)
05:51:27.82 +45:11:28.1 -- not an asteroid (will add it to exclusion list)
05:53:04.76 +46:58:02.0 -- not an asteroid (will add it to exclusion list)
05:42:47.66 +50:22:59.9 -- not an asteroid (will add it to exclusion list)
06:35:26.95 +44:24:50.4 -- not an asteroid (will add it to exclusion list)
06:14:03.05 +50:52:47.6 -- not an asteroid (will add it to exclusion list)
05:46:41.19 +49:10:47.8 -- not an asteroid (will add it to exclusion list)
05:39:45.66 +44:56:08.8 -- not an asteroid (will add it to exclusion list)
05:49:04.53 +41:17:27.2 -- not an asteroid (will add it to exclusion list)
06:02:31.73 +46:29:05.9 -- not an asteroid (will add it to exclusion list)
06:04:53.14 +50:08:48.5 -- not an asteroid (will add it to exclusion list)
06:02:14.09 +47:47:00.1 -- not an asteroid (will add it to exclusion list)
06:21:31.91 +41:49:30.9 -- not an asteroid (will add it to exclusion list)
05:54:06.60 +41:46:10.4 -- not an asteroid (will add it to exclusion list)
05:36:11.28 +43:24:36.5 -- not an asteroid (will add it to exclusion list)
05:28:04.10 +49:28:29.9 -- not an asteroid (will add it to exclusion list)
05:38:27.37 +41:13:50.9 -- not an asteroid (will add it to exclusion list)
06:20:12.78 +43:38:52.8 -- not an asteroid (will add it to exclusion list)
05:57:09.01 +46:13:43.3 -- not an asteroid (will add it to exclusion list)
05:17:54.81 +41:11:55.2 -- not an asteroid (will add it to exclusion list)
05:37:22.99 +46:49:18.2 -- not an asteroid (will add it to exclusion list)
05:25:37.69 +45:40:56.6 -- not an asteroid (will add it to exclusion list)
06:02:11.23 +46:42:58.2 -- not an asteroid (will add it to exclusion list)
06:21:48.08 +46:46:31.6 -- not an asteroid (will add it to exclusion list)
05:29:21.92 +51:11:33.0 -- not an asteroid (will add it to exclusion list)
05:40:02.91 +50:02:04.5 -- not an asteroid (will add it to exclusion list)
05:48:45.93 +46:35:01.2 -- not an asteroid (will add it to exclusion list)
05:51:18.29 +46:14:40.9 -- not an asteroid (will add it to exclusion list)
05:48:04.06 +43:19:50.4 -- not an asteroid (will add it to exclusion list)
05:28:43.85 +41:18:08.9 -- not an asteroid (will add it to exclusion list)
06:26:19.86 +41:59:11.1 -- not an asteroid (will add it to exclusion list)
05:28:01.23 +48:14:57.8 -- not an asteroid (will add it to exclusion list)
05:48:00.92 +50:37:40.6 -- not an asteroid (will add it to exclusion list)
05:35:42.14 +42:29:13.7 -- not an asteroid (will add it to exclusion list)
05:46:10.04 +46:54:48.0 -- not an asteroid (will add it to exclusion list)
05:51:03.49 +47:53:56.1 -- not an asteroid (will add it to exclusion list)
05:38:24.31 +42:59:48.0 -- not an asteroid (will add it to exclusion list)
05:28:11.70 +43:27:56.1 -- not an asteroid (will add it to exclusion list)
05:31:00.44 +42:54:52.6 -- not an asteroid (will add it to exclusion list)
05:18:50.14 +41:06:32.4 -- not an asteroid (will add it to exclusion list)
06:07:29.96 +46:55:56.8 -- not an asteroid (will add it to exclusion list)
05:48:23.18 +49:46:57.8 -- not an asteroid (will add it to exclusion list)
06:25:48.90 +48:15:43.2 -- not an asteroid (will add it to exclusion list)
05:27:26.03 +44:48:51.3 -- not an asteroid (will add it to exclusion list)
05:27:50.99 +42:20:24.9 -- not an asteroid (will add it to exclusion list)
05:22:47.43 +47:00:53.7 -- not an asteroid (will add it to exclusion list)
05:20:50.90 +44:04:36.6 -- not an asteroid (will add it to exclusion list)
05:57:45.30 +45:54:52.2 -- not an asteroid (will add it to exclusion list)
05:37:28.33 +42:00:46.1 -- not an asteroid (will add it to exclusion list)
05:40:57.34 +41:07:45.3 -- not an asteroid (will add it to exclusion list)
05:36:14.40 +43:32:31.4 -- not an asteroid (will add it to exclusion list)
06:12:44.88 +47:30:43.0 -- not an asteroid (will add it to exclusion list)
05:44:39.75 +43:57:55.6 -- not an asteroid (will add it to exclusion list)
06:13:29.68 +41:58:06.6 -- not an asteroid (will add it to exclusion list)
05:35:36.13 +47:32:42.0 -- not an asteroid (will add it to exclusion list)
06:40:19.79 +44:20:22.7 -- not an asteroid (will add it to exclusion list)
05:53:51.64 +50:42:48.8 -- not an asteroid (will add it to exclusion list)
05:37:16.23 +44:02:46.1 -- not an asteroid (will add it to exclusion list)
05:51:18.88 +43:17:46.0 -- not an asteroid (will add it to exclusion list)
05:37:19.32 +44:51:38.1 -- not an asteroid (will add it to exclusion list)
06:02:32.03 +48:11:24.7 -- not an asteroid (will add it to exclusion list)
06:00:04.54 +45:58:32.6 -- not an asteroid (will add it to exclusion list)
06:23:05.38 +49:11:45.9 -- not an asteroid (will add it to exclusion list)
06:01:16.78 +47:35:44.8 -- not an asteroid (will add it to exclusion list)
05:42:16.22 +43:16:25.6 -- not an asteroid (will add it to exclusion list)
05:38:36.16 +49:43:22.4 -- not an asteroid (will add it to exclusion list)
06:26:29.81 +49:54:10.2 -- not an asteroid (will add it to exclusion list)
05:48:07.92 +49:40:41.4 -- not an asteroid (will add it to exclusion list)
06:00:41.16 +40:57:37.0 -- not an asteroid (will add it to exclusion list)
05:49:15.53 +45:41:16.2 -- not an asteroid (will add it to exclusion list)
05:57:12.02 +42:33:32.7 -- not an asteroid (will add it to exclusion list)
06:13:27.72 +45:03:37.2 -- not an asteroid (will add it to exclusion list)
05:38:59.89 +47:35:32.0 -- not an asteroid (will add it to exclusion list)
06:07:54.28 +45:58:48.7 -- not an asteroid (will add it to exclusion list)
05:34:15.83 +44:17:05.5 -- not an asteroid (will add it to exclusion list)
05:31:08.96 +50:39:12.8 -- not an asteroid (will add it to exclusion list)
05:37:52.47 +43:02:34.3 -- not an asteroid (will add it to exclusion list)
05:48:10.11 +45:27:38.2 -- not an asteroid (will add it to exclusion list)
05:59:26.46 +46:32:41.8 -- not an asteroid (will add it to exclusion list)
05:34:18.90 +44:27:44.5 -- not an asteroid (will add it to exclusion list)
05:57:12.02 +47:27:16.4 -- not an asteroid (will add it to exclusion list)
06:14:21.48 +43:11:50.6 -- not an asteroid (will add it to exclusion list)
05:36:40.83 +50:02:55.4 -- not an asteroid (will add it to exclusion list)
06:10:45.05 +48:16:57.3 -- not an asteroid (will add it to exclusion list)
05:50:43.76 +46:21:03.3 -- not an asteroid (will add it to exclusion list)
06:05:19.87 +49:43:46.5 -- not an asteroid (will add it to exclusion list)
06:25:47.98 +49:52:45.3 -- not an asteroid (will add it to exclusion list)
06:38:58.52 +48:06:11.7 -- not an asteroid (will add it to exclusion list)
05:56:05.19 +44:35:31.1 -- not an asteroid (will add it to exclusion list)
06:20:46.17 +50:02:59.8 -- not an asteroid (will add it to exclusion list)
06:41:34.47 +49:47:47.0 -- not an asteroid (will add it to exclusion list)
05:57:28.48 +47:42:20.7 -- not an asteroid (will add it to exclusion list)
05:33:27.71 +48:41:06.2 -- not an asteroid (will add it to exclusion list)
05:39:25.73 +43:54:06.0 -- not an asteroid (will add it to exclusion list)
06:25:16.30 +45:04:14.5 -- not an asteroid (will add it to exclusion list)
06:06:36.45 +47:00:44.4 -- not an asteroid (will add it to exclusion list)
05:56:44.19 +47:22:14.9 -- not an asteroid (will add it to exclusion list)
06:09:51.91 +46:34:27.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:16:30.21 +45:55:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:54.81 +41:11:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:50.14 +41:06:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.90 +44:04:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:47.43 +47:00:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.69 +45:40:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.81 +50:07:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.03 +44:48:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:50.99 +42:20:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.23 +48:14:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.10 +49:28:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.70 +43:27:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:43.85 +41:18:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:21.92 +51:11:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:00.44 +42:54:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:08.96 +50:39:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:27.71 +48:41:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.83 +44:17:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:18.90 +44:27:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:36.13 +47:32:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:42.14 +42:29:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:11.28 +43:24:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:14.40 +43:32:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.83 +50:02:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.23 +44:02:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.32 +44:51:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:22.99 +46:49:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:28.33 +42:00:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.47 +43:02:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:24.31 +42:59:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.37 +41:13:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:36.16 +49:43:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:59.89 +47:35:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:25.73 +43:54:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:45.66 +44:56:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.91 +50:02:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:57.34 +41:07:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:16.22 +43:16:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:47.66 +50:22:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:39.75 +43:57:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:10.04 +46:54:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:41.19 +49:10:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:00.92 +50:37:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.06 +43:19:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:07.92 +49:40:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:10.11 +45:27:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.18 +49:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:45.93 +46:35:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:04.53 +41:17:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:15.53 +45:41:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:43.76 +46:21:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:03.49 +47:53:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.29 +46:14:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.88 +43:17:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:27.82 +45:11:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.76 +46:58:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:51.64 +50:42:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:06.60 +41:46:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:05.19 +44:35:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:44.19 +47:22:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:09.01 +46:13:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.02 +42:33:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.02 +47:27:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:28.48 +47:42:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:45.30 +45:54:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:26.46 +46:32:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:04.54 +45:58:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:41.16 +40:57:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.78 +47:35:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:11.23 +46:42:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.09 +47:47:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:31.73 +46:29:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.03 +48:11:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:53.14 +50:08:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:19.87 +49:43:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:36.45 +47:00:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:29.96 +46:55:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.28 +45:58:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.91 +46:34:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.05 +48:16:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:44.88 +47:30:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:27.72 +45:03:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.68 +41:58:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:03.05 +50:52:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:21.48 +43:11:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:12.78 +43:38:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:46.17 +50:02:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.91 +41:49:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.08 +46:46:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:05.38 +49:11:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:16.30 +45:04:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:47.98 +49:52:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:48.90 +48:15:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.86 +41:59:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.81 +49:54:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:26.95 +44:24:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:58.52 +48:06:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:19.79 +44:20:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:34.47 +49:47:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:16:30.21 +45:55:23.3 -- not a known variable star
05:17:54.81 +41:11:55.2 -- a known variable star
05:18:50.14 +41:06:32.4 -- not a known variable star
05:20:50.90 +44:04:36.6 -- not a known variable star
05:22:47.43 +47:00:53.7 -- not a known variable star
05:25:37.69 +45:40:56.6 -- not a known variable star
05:27:04.81 +50:07:23.9 -- a known variable star
05:27:26.03 +44:48:51.3 -- not a known variable star
05:27:50.99 +42:20:24.9 -- not a known variable star
05:28:01.23 +48:14:57.8 -- a known variable star
05:28:04.10 +49:28:29.9 -- not a known variable star
05:28:11.70 +43:27:56.1 -- not a known variable star
05:28:43.85 +41:18:08.9 -- not a known variable star
05:29:21.92 +51:11:33.0 -- not a known variable star
05:31:00.44 +42:54:52.6 -- not a known variable star
05:31:08.96 +50:39:12.8 -- not a known variable star
05:33:27.71 +48:41:06.2 -- not a known variable star
05:34:15.83 +44:17:05.5 -- not a known variable star
05:34:18.90 +44:27:44.5 -- not a known variable star
05:35:36.13 +47:32:42.0 -- not a known variable star
05:35:42.14 +42:29:13.7 -- not a known variable star
05:36:11.28 +43:24:36.5 -- a known variable star
05:36:14.40 +43:32:31.4 -- not a known variable star
05:36:40.83 +50:02:55.4 -- not a known variable star
05:37:16.23 +44:02:46.1 -- not a known variable star
05:37:19.32 +44:51:38.1 -- not a known variable star
05:37:22.99 +46:49:18.2 -- not a known variable star
05:37:28.33 +42:00:46.1 -- not a known variable star
05:37:52.47 +43:02:34.3 -- not a known variable star
05:38:24.31 +42:59:48.0 -- not a known variable star
05:38:27.37 +41:13:50.9 -- not a known variable star
05:38:36.16 +49:43:22.4 -- not a known variable star
05:38:59.89 +47:35:32.0 -- not a known variable star
05:39:25.73 +43:54:06.0 -- a known variable star
05:39:45.66 +44:56:08.8 -- not a known variable star
05:40:02.91 +50:02:04.5 -- not a known variable star
05:40:57.34 +41:07:45.3 -- a known variable star
05:42:16.22 +43:16:25.6 -- not a known variable star
05:42:47.66 +50:22:59.9 -- not a known variable star
05:44:39.75 +43:57:55.6 -- not a known variable star
05:46:10.04 +46:54:48.0 -- a known variable star
05:46:41.19 +49:10:47.8 -- not a known variable star
05:48:00.92 +50:37:40.6 -- not a known variable star
05:48:04.06 +43:19:50.4 -- not a known variable star
05:48:07.92 +49:40:41.4 -- not a known variable star
05:48:10.11 +45:27:38.2 -- not a known variable star
05:48:23.18 +49:46:57.8 -- not a known variable star
05:48:45.93 +46:35:01.2 -- a known variable star
05:49:04.53 +41:17:27.2 -- not a known variable star
05:49:15.53 +45:41:16.2 -- not a known variable star
05:50:43.76 +46:21:03.3 -- not a known variable star
05:51:03.49 +47:53:56.1 -- not a known variable star
05:51:18.29 +46:14:40.9 -- not a known variable star
05:51:18.88 +43:17:46.0 -- not a known variable star
05:51:27.82 +45:11:28.1 -- a known variable star
05:53:04.76 +46:58:02.0 -- not a known variable star
05:53:51.64 +50:42:48.8 -- not a known variable star
05:54:06.60 +41:46:10.4 -- a known variable star
05:56:05.19 +44:35:31.1 -- not a known variable star
05:56:44.19 +47:22:14.9 -- not a known variable star
05:57:09.01 +46:13:43.3 -- not a known variable star
05:57:12.02 +42:33:32.7 -- not a known variable star
05:57:12.02 +47:27:16.4 -- not a known variable star
05:57:28.48 +47:42:20.7 -- not a known variable star
05:57:45.30 +45:54:52.2 -- not a known variable star
05:59:26.46 +46:32:41.8 -- not a known variable star
06:00:04.54 +45:58:32.6 -- not a known variable star
06:00:41.16 +40:57:37.0 -- not a known variable star
06:01:16.78 +47:35:44.8 -- not a known variable star
06:02:11.23 +46:42:58.2 -- not a known variable star
06:02:14.09 +47:47:00.1 -- a known variable star
06:02:31.73 +46:29:05.9 -- not a known variable star
06:02:32.03 +48:11:24.7 -- not a known variable star
06:04:53.14 +50:08:48.5 -- not a known variable star
06:05:19.87 +49:43:46.5 -- not a known variable star
06:06:36.45 +47:00:44.4 -- not a known variable star
06:07:29.96 +46:55:56.8 -- not a known variable star
06:07:54.28 +45:58:48.7 -- not a known variable star
06:09:51.91 +46:34:27.7 -- a known variable star
06:10:45.05 +48:16:57.3 -- not a known variable star
06:12:44.88 +47:30:43.0 -- not a known variable star
06:13:27.72 +45:03:37.2 -- a known variable star
06:13:29.68 +41:58:06.6 -- not a known variable star
06:14:03.05 +50:52:47.6 -- not a known variable star
06:14:21.48 +43:11:50.6 -- not a known variable star
06:20:12.78 +43:38:52.8 -- a known variable star
06:20:46.17 +50:02:59.8 -- a known variable star
06:21:31.91 +41:49:30.9 -- not a known variable star
06:21:48.08 +46:46:31.6 -- not a known variable star
06:23:05.38 +49:11:45.9 -- not a known variable star
06:25:16.30 +45:04:14.5 -- a known variable star
06:25:47.98 +49:52:45.3 -- not a known variable star
06:25:48.90 +48:15:43.2 -- not a known variable star
06:26:19.86 +41:59:11.1 -- not a known variable star
06:26:29.81 +49:54:10.2 -- not a known variable star
06:35:26.95 +44:24:50.4 -- not a known variable star
06:38:58.52 +48:06:11.7 -- not a known variable star
06:40:19.79 +44:20:22.7 -- not a known variable star
06:41:34.47 +49:47:47.0 -- not a known variable star
Found 83 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
99 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 99 (excluding asteroids and hot pixels, 83 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)2461144.63689470 -observatory V36
23:57:35.93 -03:03:08.8 Mercury (0.1mag)
02:59:33.60 +17:08:49.0 Venus (-3.9mag)
00:12:32.81 +00:16:55.6 Mars (1.2mag)
07:11:48.13 +22:47:35.1 Jupiter (-2.1mag)
00:28:20.95 +00:43:47.3 Saturn (0.9mag)
03:47:18.45 +19:46:13.6 Uranus (5.8mag)
00:10:35.74 -00:16:54.8 Neptune (7.8mag)
20:33:40.19 -22:52:31.4 Pluto (14.5mag)
22:44:08.01 -08:08:47.1 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 13 22:21 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.63689470:
07:11:43.81 +22:47:45.9 Io (5.8mag)
07:11:47.58 +22:47:33.1 Europa (5.9mag)
07:11:56.10 +22:47:25.3 Ganymede (5.3mag)
07:12:14.16 +22:46:49.0 Callisto (6.6mag)
07:15:13.19 +22:36:05.2 Himalia (15.3mag)
07:11:45.02 +22:47:40.3 Thebe (16.2mag)
07:15:22.15 +23:06:07.7 Elara (17.3mag)
07:10:33.40 +23:28:33.9 Pasiphae (17.4mag)
07:20:10.29 +22:45:25.2 Carme (18.5mag)
00:28:29.05 +00:44:03.3 Titan (8.8mag)
00:28:23.27 +00:44:00.8 Rhea (10.1mag)
00:28:04.33 +00:44:14.6 Iapetus (11.5mag)
00:28:34.31 +00:43:56.0 Hyperion (14.8mag)
00:29:59.32 +00:52:47.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 22:21 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.63689470:
15:30:00.22 -14:54:16.0 JWST
16:58:48.78 +44:40:32.2 Chandra
07:53:57.91 -35:11:23.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 22:21 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.63689470 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:13.13 -28:40:13.6 13.9mag P/2010 H2 (Vales)
05:05:24.42 -69:45:02.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:02.96 +31:25:29.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.45 +10:19:35.6 17.6mag C/2021 G2 (ATLAS)
23:09:43.31 +29:09:20.3 17.1mag C/2022 E2 (ATLAS)
04:27:04.14 +25:59:15.9 16.0mag C/2022 N2 (PANSTARRS)
09:03:02.04 +32:00:19.7 16.2mag C/2022 QE78 (ATLAS)
08:30:47.82 -00:21:04.7 17.3mag C/2022 R6 (PANSTARRS)
18:54:09.75 +18:22:32.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:16.23 -11:32:55.7 17.5mag P/2023 B1 (PANSTARRS)
09:08:30.83 -12:10:57.8 17.6mag C/2023 F3 (ATLAS)
21:52:19.39 +62:47:53.0 17.5mag C/2023 H5 (Lemmon)
19:20:46.66 -03:42:10.1 14.2mag C/2023 R1 (PANSTARRS)
21:35:56.57 +85:39:14.8 17.8mag C/2023 X2 (Lemmon)
06:17:03.41 +63:31:19.1 17.1mag C/2024 A1 (ATLAS)
05:09:15.06 +17:40:35.9 10.9mag C/2024 E1 (Wierzchos)
16:20:27.84 +06:05:05.9 17.4mag C/2024 G6 (ATLAS)
20:20:16.67 +14:46:11.8 14.6mag C/2024 J3 (ATLAS)
03:24:41.95 -22:40:12.3 16.4mag C/2024 T5 (ATLAS)
05:15:08.24 +45:45:21.7 17.7mag C/2025 J1 (Borisov)
13:46:34.91 +44:13:48.4 15.1mag C/2025 L1 (ATLAS)
03:22:20.57 -25:55:21.2 17.8mag C/2025 Q3 (ATLAS)
23:28:31.04 +19:09:01.3 8.8mag C/2025 R3 (PANSTARRS)
12:54:55.62 +02:53:56.3 17.4mag C/2025 Y1 (ATLAS)
03:11:51.62 +02:50:21.1 12.7mag C/2026 A1 (MAPS)
23:54:16.39 +36:52:21.7 14.5mag C/2026 B2 (Sun-Gao)
18:39:18.46 -09:49:06.6 11.9mag 10P/Tempel
15:02:49.38 +03:24:01.8 13.8mag 24P/Schaumasse
11:03:18.50 -01:35:11.9 15.7mag 29P/Schwassmann-Wachmann
18:00:23.61 -09:40:44.9 17.9mag 40P/Vaisala
10:37:39.75 -04:14:54.5 16.9mag 43P/Wolf-Harrington
01:45:47.36 +17:10:11.1 17.2mag 47P/Ashbrook-Jackson
07:07:20.26 +37:24:45.4 17.0mag 63P/Wild
23:26:40.54 -11:40:30.5 15.7mag 65P/Gunn
03:58:16.91 +20:36:42.3 15.9mag 76P/West-Kohoutek-Ikemura
01:01:27.44 +07:51:44.2 14.3mag 78P/Gehrels
22:57:20.67 -09:56:31.4 14.6mag 88P/Howell
02:05:08.14 +20:08:38.7 15.1mag 93P/Lovas
04:51:18.11 +32:11:16.3 16.2mag 123P/West-Hartley
08:26:11.50 +39:13:16.0 16.2mag 124P/Mrkos
02:30:20.26 +14:09:42.8 16.4mag 128P/Shoemaker-Holt
02:43:52.94 +14:15:54.7 17.5mag 131P/Mueller
01:16:23.78 +12:35:20.5 10.7mag 141P/Machholz
01:25:34.83 +04:10:27.5 10.7mag 141P-A/Machholz
00:11:46.94 +00:09:13.6 13.0mag 141P-D/Machholz
01:55:44.80 +05:55:37.4 17.8mag 141P-I/Machholz
00:57:10.91 -02:27:45.6 15.1mag 162P/SidingSpring
10:29:06.39 +30:57:36.6 18.0mag 164P/Christensen
06:33:05.13 +24:18:02.5 18.0mag 198P/ODAS
14:54:44.89 -00:15:46.1 17.6mag 210P/Christensen
21:33:25.38 -11:53:52.6 17.6mag 218P/LINEAR
17:16:04.08 -14:09:23.5 16.1mag 235P/LINEAR
05:30:27.78 +34:33:21.2 16.7mag 240P/NEAT
07:37:35.26 -05:22:12.1 17.7mag 242P/Spahr
22:12:15.05 -21:28:21.4 17.9mag 260P/McNaught
15:43:21.69 +06:52:01.0 17.5mag 391P/Kowalski
07:33:29.38 +21:21:35.5 17.7mag 450P/LONEOS
05:33:09.49 +45:08:30.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 22:21 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
-rw-r--r-- 1 apache apache 5.8K Apr 13 22:21 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 13 22:21 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
20:29:30.119 -10:56:33.33 AT 2026iuw 2026-03-29.79 19.55
13:31:30.960 -32:00:09.92 AT 2026iuv 2026-04-07.60 18.91
14:00:56.468 -25:06:29.29 AT 2026iuu 2026-04-07.35 18.482
13:27:25.132 +09:30:53.72 AT 2026iut 2026-04-05.33 19.4971
13:57:28.106 -31:36:18.49 AT 2026ius 2026-04-07.61 19.27
09:54:32.050 -01:17:25.84 SN 2026iur 2026-04-07.01 15.9
14:24:08.131 +22:56:14.71 AT 2026iuq 2026-04-07.38 19.91
10:07:28.221 -17:12:04.00 AT 2026iup 2026-04-05.31 20.26
16:21:33.361 +42:39:39.49 AT 2026iuo 2026-04-02.59 20.72
11:27:41.500 -35:48:12.21 AT 2026iun 2026-03-30.51 19.56
13:57:31.503 -10:38:39.68 AT 2026ium 2026-03-29.71 19.95
19:51:44.150 +31:28:49.50 AT 2026iul 2026-04-07.40 15.7
-rw-r--r-- 1 apache apache 30K Apr 13 22:21 tns_transients_list.txt
