This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SY Mon,2461144.6066,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SY Mon 20260414.1066 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0253-01.9062,2461144.6066,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0253-01.9062 20260414.1066 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6066,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8499-02.8303,2461144.6066,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8499-02.8303 20260414.1066 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125569957548660864,2461144.6066,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125569957548660864 20260414.1066 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101503262931006720,2461144.6066,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503262931006720 20260414.1066 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 3101486289219649920,2461144.6066,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101486289219649920 20260414.1066 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112640181842895232,2461144.6066,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112640181842895232 20260414.1066 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6113+01.8654,2461144.6066,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6113+01.8654 20260414.1066 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461144.6066,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114694099624336256 20260414.1066 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107928495341091456,2461144.6066,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107928495341091456 20260414.1066 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2433-00.4249,2461144.6066,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2433-00.4249 20260414.1066 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109471389332247552,2461144.6066,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109471389332247552 20260414.1066 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070621.56-015037.5,2461144.6066,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J070621.56-015037.5 20260414.1066 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053389149496017280,2461144.6066,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053389149496017280 20260414.1066 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108634145589904768,2461144.6066,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108634145589904768 20260414.1066 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3280-03.1171,2461144.6066,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3280-03.1171 20260414.1066 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
ATO J105.3094-02.1493,2461144.6066,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3094-02.1493 20260414.1066 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
ATO J106.4642-01.1247,2461144.6066,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4642-01.1247 20260414.1066 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6066,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107988968482458496,2461144.6066,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107988968482458496 20260414.1066 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1626-04.9704,2461144.6066,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1626-04.9704 20260414.1066 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6066,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070631.45-055958.0,2461144.6066,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J070631.45-055958.0 20260414.1066 12.23CV 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 3112749274012032640,2461144.6066,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112749274012032640 20260414.1066 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5007-03.7484,2461144.6066,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5007-03.7484 20260414.1066 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.4234-01.2112,2461144.6066,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4234-01.2112 20260414.1066 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107714060519716992,2461144.6066,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107714060519716992 20260414.1066 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112551941736184448,2461144.6066,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112551941736184448 20260414.1066 12.30CV 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 J107.1845-01.7588,2461144.6066,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1845-01.7588 20260414.1066 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9567-01.5879,2461144.6066,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9567-01.5879 20260414.1066 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101628912187905408,2461144.6066,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101628912187905408 20260414.1066 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
target,2461144.6066,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070804.67-033414.7,2461144.6066,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J070804.67-033414.7 20260414.1066 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113577274989419904,2461144.6066,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113577274989419904 20260414.1066 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9816-06.0164,2461144.6066,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9816-06.0164 20260414.1066 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
ATO J105.6319-03.4457,2461144.6066,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.6319-03.4457 20260414.1066 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108710218049617536,2461144.6066,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108710218049617536 20260414.1066 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
target,2461144.6066,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107580676014313728,2461144.6066,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107580676014313728 20260414.1066 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
Gaia DR3 3113846517899106816,2461144.6066,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113846517899106816 20260414.1066 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109532137349277568,2461144.6066,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109532137349277568 20260414.1066 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
target,2461144.6066,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 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
target,2461144.6066,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0172-01.7704,2461144.6066,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0172-01.7704 20260414.1066 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2256-01.7850,2461144.6066,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2256-01.7850 20260414.1066 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
Gaia DR3 3108979667116800384,2461144.6066,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108979667116800384 20260414.1066 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6066,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103981287255761536,2461144.6066,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103981287255761536 20260414.1066 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461144.6066,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112424230887731712 20260414.1066 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112882349279538816,2461144.6066,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112882349279538816 20260414.1066 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1134-00.1178,2461144.6066,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1134-00.1178 20260414.1066 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.4580-02.6934,2461144.6066,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.4580-02.6934 20260414.1066 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EG Mon,2461144.6066,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EG Mon 20260414.1066 9.40CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0643204+020852,2461144.6066,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0643204+020852 20260414.1066 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J063800.58-001324.1,2461144.6066,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063800.58-001324.1 20260414.1066 12.27CV 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,2461144.6066,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1066 11.72CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Mon,2461144.6066,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Mon 20260414.1066 11.54CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0643141-003633,2461144.6066,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0643141-003633 20260414.1066 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461144.60701550 14.04.2026 02:33:56.139 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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): 28885
Objects passed selection criteria: 28742
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 20775.5
Average stars matched: 18964.5 (91.283 %)
Memory usage VmPeak: 131292 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 21:37:29 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461144.60701550 14.04.2026 02:33:56.139 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 178
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 96 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): 212133
Objects passed selection criteria: 211431
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 151959
Average stars matched: 138218 (90.9576 %)
Memory usage VmPeak: 1955560 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 21:43:00 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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: 2461144.60625929
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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.689 -02:00:05.40
Angular distance between the image centers 0.0725 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:29.041 -01:59:53.53
Angular distance between the image centers 0.0588 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 06:51:25.689 -02:00:05.40
Second-epoch second image center 06:51:29.041 -01:59:53.53
Angular distance between the image centers 0.01434 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.xgx6DDv9tQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.TGYTcMsZil
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits &> /tmp/tmp.DYyEbDATCz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits &> /tmp/tmp.ardLBhNQoZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.3 (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.xgx6DDv9tQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.TGYTcMsZil (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DYyEbDATCz (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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1381, passed=17541
Got 17541 stars (including 16149 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat
util/solve_plate_with_UCAC5 got 17541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
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: 929 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 17169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 413 to 468 (Dec -7.3 to 3.4)
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: 930 matched stars entering correct_measured_positions(), 17171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 17171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 930 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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.ardLBhNQoZ (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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1312, passed=16949
Got 16949 stars (including 15623 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat
util/solve_plate_with_UCAC5 got 16949 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 16498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 933 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(), 16502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 16501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 929 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21092.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53885_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 53885_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:09:13.69 -02:21:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21092_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 21092_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06678_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 06678_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:35:46.87 -05:22:33.7 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:37:31.62 -01:23:42.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.689 -02:00:05.40
Angular distance between the image centers 0.0725 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:29.041 -01:59:53.53
Angular distance between the image centers 0.0588 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 06:51:25.689 -02:00:05.40
Second-epoch second image center 06:51:29.041 -01:59:53.53
Angular distance between the image centers 0.01434 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.WkuXsIZ5Ij
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.OakV1f65gp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits &> /tmp/tmp.Be6reKYDHE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits &> /tmp/tmp.sFCYtUvNPi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 154 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WkuXsIZ5Ij (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.OakV1f65gp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Be6reKYDHE (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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=13869, passed=115953
Got 115953 stars (including 101990 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat
util/solve_plate_with_UCAC5 got 115953 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 113442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 113442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 113444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 924 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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.sFCYtUvNPi (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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=13360, passed=112717
Got 112717 stars (including 99270 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat
util/solve_plate_with_UCAC5 got 112717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 109555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 109559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 109580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-32-50_20.00sec_-4.90C_LIGHT_0642.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.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_Mon-02-Q2b1x1_213500_TTUQ2b1x1_8241_PLoVoLo5/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out237671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out304064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out304149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out304527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out304673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out306146.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out169635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out221821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80449.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 73s
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: 41s
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Considering the candidate 283503_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283503_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283504_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283504_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:52.30 -00:44:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.210 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283522_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283522_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283523_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283523_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283529_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283529_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283533_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283533_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283534_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283534_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283542_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283542_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283545_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283545_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 283558_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283558_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283563_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:42:23.12 +01:21:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 5.433 3125888884639350784 100.59608866886 +01.35242739877 12.8037 11.2981 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283566_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283566_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:51:02.44 +01:07:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283578_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283578_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283579_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283579_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283580_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283580_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:54:08.15 -05:53:03.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 283581_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283581_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:52:13.42 -00:19:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283584_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283584_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283586_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283586_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:07:01.70 -01:48:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.021 3109255094780895872 106.75660645148 -01.81640793452 12.8006 12.0355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283589_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283589_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 283590_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283590_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:05:11.16 -00:29:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.731 3112693400776779520 106.29629603399 -00.48935224730 12.8501 12.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283591_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283591_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:36.72 -01:40:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283592_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 283592_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283597_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283597_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:13.87 -03:36:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283601_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283601_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:09:18.40 -01:42:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.616 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283603_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283603_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:48.32 +00:19:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.542 3114274601576731904 107.20115234593 +00.32769523318 12.5229 11.7962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283605_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283605_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:51:44.51 +00:29:60.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:07:26.05 -01:50:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283609_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283609_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:58:26.68 -00:54:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283611_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 283611_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:07:49.50 -05:43:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288259_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 288259_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:50:40.22 -00:32:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290890_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 290890_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:37.97 -05:29:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291558_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 291558_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:40:30.67 -01:04:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291708_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 291708_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:51:39.73 +00:25:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292102_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 292102_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:10.70 -03:14:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293668_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 293668_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:02:11.31 -06:02:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295372_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 295372_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:07:16.70 -04:03:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295907_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 295907_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:05:52.45 -01:02:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296211_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 296211_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:50:41.66 -00:33:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297322_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 297322_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:52:25.52 -05:17:26.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298865_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 298865_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:52.76 -01:19:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299198_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 299198_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:10.58 +00:02:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.559 3112774390980328320 106.04409922559 +00.04009490383 12.8697 12.0978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299573_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 299573_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299575_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 299575_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:02:39.69 -04:37:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 299608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299687_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 299687_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:53:08.20 -04:35:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300003_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 300003_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:36:41.06 -05:13:18.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300050_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 300050_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:09:22.85 -04:08:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.753 3107533946769387392 107.34498467445 -04.14990516113 12.9877 12.2399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300502_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 300502_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:17.21 +00:25:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.470 3114280099135354112 107.07174264372 +00.43204080684 12.8009 11.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300685_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 300685_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300686_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 300686_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300716_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 300716_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300772_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 300772_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:09:37.57 -01:22:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.926 3109339379218885888 107.40665275024 -01.37683283674 13.0624 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301252_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 301252_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:51.39 -01:46:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.939 3109234234118285952 107.21394667394 -01.77617496224 13.0380 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301319_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 301319_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:18.51 -03:02:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.090 3108655929664211072 106.07666031661 -03.03495984401 13.0643 12.6085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301689_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 301689_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301855_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 301855_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:02:22.94 +00:25:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.565 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301860_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 301860_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302115_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 302115_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:00:50.47 -04:30:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.831 3101735908414140416 105.20979162595 -04.51016365204 12.8843 12.0606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302423_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 302423_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:03:41.84 -00:34:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.892 3112600358906822784 105.92435322766 -00.57610862188 12.3354 11.1129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302523_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 302523_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303228_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303228_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:54:30.12 -04:07:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303239_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303239_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:54:09.40 -05:52:27.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303562_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303562_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:06:52.41 -00:27:18.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 303608_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303633_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303633_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:00:06.71 -02:51:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303647_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303647_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:50:44.58 -00:31:40.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 303989_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 303989_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 303993_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 303993_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:32.39 -05:17:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.412 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304064_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 304064_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:23.73 +00:30:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.866 3114292571720574464 107.09853168373 +00.50913942528 13.2073 12.2839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304149_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 304149_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:07:58.63 -00:56:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.779 3109605186152914432 106.99387176228 -00.94487186150 13.3450 12.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304527_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 304527_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:59:50.08 +00:16:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.467 3112948006440304640 104.95896919067 +00.27146844100 13.2300 12.8150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304673_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 304673_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:43.65 -00:29:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.367 3112692889681609088 106.18162536672 -00.49277504927 13.1660 12.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304681_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 304681_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 305087_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 305087_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:45:00.26 -00:03:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305118_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305118_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 305175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 305175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:02:47.97 -04:14:39.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 305232_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305232_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305319_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 305319_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:00:21.40 -05:50:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.658 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305450_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305450_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 305497_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305497_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305748_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 305748_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:56:45.70 +00:46:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305801_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305801_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 305949_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 305949_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 306033_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306033_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306066_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 306066_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:44.73 -00:27:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.812 3112693125898976128 106.18617333971 -00.46329564351 13.2235 12.3843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306146_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 306146_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:59:02.57 -03:29:53.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
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Considering the candidate 306185_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306185_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 306283_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306283_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306327_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306327_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 306627_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306627_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 306863_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 306863_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 307175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307407_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 307407_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:56:27.60 +00:06:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.064 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307610_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 307610_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:58:38.92 -04:20:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.921 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307647_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 307647_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 307650_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 307650_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:22.86 -06:08:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.508 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307976_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 307976_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308165_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 308165_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:43:50.08 +01:35:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308264_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 308264_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308383_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 308383_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 308743_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 308743_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 308784_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 308784_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:00.62 -03:17:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.275 3107890532129879680 106.00168451418 -03.29622223652 13.4503 12.6854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309003_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 309003_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309032_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 309032_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:53.90 -03:51:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.082 3107694853426314624 107.22456365729 -03.86588354665 13.3330 12.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309055_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 309055_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309077_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 309077_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:22.46 -03:06:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309265_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 309265_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:51.42 -02:16:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.975 3108857002851931776 106.21398983457 -02.28187184212 13.3926 12.6907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309496_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 309496_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:00:51.71 -03:52:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.434 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310053_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 310053_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:37:58.54 -01:25:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310198_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 310198_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 310229_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 310229_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310248_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 310248_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310492_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 310492_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:03:39.62 -00:16:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.919 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310588_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 310588_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:00:53.60 +02:12:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.820 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310646_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 310646_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 310962_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 310962_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:45:04.89 -01:02:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.342 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 311175_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 311213_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 311213_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:04:34.69 -05:56:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311278_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 311278_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 311991_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 311991_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 312111_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 312111_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:00.08 -00:57:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.617 3109605181852110976 107.00017650752 -00.95349251268 13.5091 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312329_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 312329_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:59:57.27 -00:05:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.707 3112885196837878016 104.98858288935 -00.08675063744 13.5793 12.7573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313074_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 313074_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 313662_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 313662_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:58:28.08 -05:44:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315640_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 315640_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 317218_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 317218_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:01:35.48 -00:48:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.862 3112578162515589760 105.39724095265 -00.80783877429 14.1459 13.7567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157311_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 157311_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:33:38.19 -01:13:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265915_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 265915_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:52:00.38 +00:12:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.050 3113357819339125504 103.00115885910 +00.20192758615 11.7103 10.0166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 80449_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 80449_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 131156_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 131156_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:05:28.50 -02:00:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:09:13.68 -02:21:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 07:08:45.32 +00:41:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47993_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 47993_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:51:26.35 -05:15:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 47889_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:44:47.61 -05:17:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57802_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 57802_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:45:42.44 -04:56:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221821_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 221821_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 179553_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 179553_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 152309_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 152309_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:37:31.61 -01:23:42.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:41:59.33 -01:11:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67235_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 67235_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:37:53.47 -05:55:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31629_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 31629_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
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Considering the candidate 237671_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 237671_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:40:09.06 +01:22:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.966 3126632974834859392 100.03692742394 +01.37171623584 12.6357 11.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:50:00.78 +01:46:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49190_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 49190_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:35:46.89 -05:22:33.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 127999_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 127999_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:49:16.34 -02:16:18.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154375_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 154375_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:48:19.06 -01:19:11.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169635_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
Preparing report for the candidate 169635_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121814_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 121814_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:38:20.55 -02:32:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107626_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 107626_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:34:21.72 -03:04:27.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 198847_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 198847_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:41:05.51 +00:29:40.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53553_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 53553_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:36:35.43 -05:12:39.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247718_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643
The candidate 247718_fd_Mon-02-Q2b1x1_2026-04-13_21-33-56_20.00sec_-4.90C_LIGHT_0643 did not pass the final checks
**** FOUND 06:35:16.01 +00:53:22.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 117s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:37:31.62 -01:23:42.9
06:43:14.27 -00:36:30.1
06:38:00.88 -00:13:22.9
06:43:20.66 +02:08:46.4
07:04:06.78 -01:54:19.1
06:40:38.83 -04:53:10.1
07:03:24.11 -02:49:51.8
06:43:16.47 +00:21:51.2
07:03:25.15 -05:00:43.3
07:05:06.40 -04:50:36.9
06:59:40.46 -00:39:47.2
06:58:26.81 +01:51:58.8
07:07:06.90 +01:39:59.6
07:06:38.32 -03:18:53.8
07:01:00.97 -00:25:44.3
07:05:18.23 -01:23:01.5
07:06:22.88 -01:50:00.4
07:05:04.34 -05:27:56.0
07:01:07.63 -03:14:32.1
07:01:19.13 -03:06:46.0
07:01:11.44 -02:08:50.1
07:05:51.51 -01:07:33.2
07:00:56.86 -03:16:18.5
07:07:11.46 -02:58:22.0
07:04:39.04 -04:57:05.7
07:08:12.65 -03:12:27.9
07:06:30.46 -06:00:02.1
07:05:14.68 +00:02:13.0
07:01:59.65 -03:44:51.2
07:05:41.86 -01:12:41.9
07:08:03.19 -03:37:55.5
07:01:50.92 -01:07:00.2
07:08:44.04 -01:45:46.0
06:55:49.94 -01:35:05.7
06:59:52.95 -04:47:26.6
06:56:45.24 +00:46:35.9
07:08:03.39 -03:34:27.0
06:52:07.78 +00:28:18.4
07:03:52.76 -06:00:22.7
07:02:31.17 -03:26:38.0
07:00:38.94 -02:48:52.4
07:01:48.91 +01:06:05.9
07:06:12.26 -04:08:44.2
06:59:39.95 +01:04:05.3
07:03:04.49 -01:18:37.5
06:54:15.95 -00:38:33.5
06:52:57.35 -03:04:56.8
07:07:59.74 -01:46:27.0
07:04:54.95 -01:47:05.8
06:57:15.16 -02:29:05.7
06:44:31.52 +00:07:36.7
06:40:17.51 -04:25:58.6
06:56:22.08 -00:53:12.5
07:01:10.26 +00:00:19.7
07:00:27.53 -00:07:02.3
06:57:52.56 -02:41:35.3
07:09:11.08 -05:50:46.7
06:40:18.84 -04:30:20.6
06:52:06.25 -04:01:50.1
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:37:31.62 -01:23:42.9
07:04:06.78 -01:54:19.1
06:40:38.83 -04:53:10.1
07:03:24.11 -02:49:51.8
06:43:16.47 +00:21:51.2
07:03:25.15 -05:00:43.3
07:05:06.40 -04:50:36.9
06:59:40.46 -00:39:47.2
06:58:26.81 +01:51:58.8
07:07:06.90 +01:39:59.6
07:06:38.32 -03:18:53.8
07:01:00.97 -00:25:44.3
07:05:18.23 -01:23:01.5
07:06:22.88 -01:50:00.4
07:05:04.34 -05:27:56.0
07:01:07.63 -03:14:32.1
07:01:19.13 -03:06:46.0
07:01:11.44 -02:08:50.1
07:05:51.51 -01:07:33.2
07:00:56.86 -03:16:18.5
07:07:11.46 -02:58:22.0
07:04:39.04 -04:57:05.7
07:08:12.65 -03:12:27.9
07:06:30.46 -06:00:02.1
07:05:14.68 +00:02:13.0
07:01:59.65 -03:44:51.2
07:05:41.86 -01:12:41.9
07:08:03.19 -03:37:55.5
07:01:50.92 -01:07:00.2
07:08:44.04 -01:45:46.0
06:55:49.94 -01:35:05.7
06:59:52.95 -04:47:26.6
06:56:45.24 +00:46:35.9
07:08:03.39 -03:34:27.0
06:52:07.78 +00:28:18.4
07:03:52.76 -06:00:22.7
07:02:31.17 -03:26:38.0
07:00:38.94 -02:48:52.4
07:01:48.91 +01:06:05.9
07:06:12.26 -04:08:44.2
06:59:39.95 +01:04:05.3
07:03:04.49 -01:18:37.5
06:54:15.95 -00:38:33.5
06:52:57.35 -03:04:56.8
07:07:59.74 -01:46:27.0
07:04:54.95 -01:47:05.8
06:57:15.16 -02:29:05.7
06:44:31.52 +00:07:36.7
06:40:17.51 -04:25:58.6
06:56:22.08 -00:53:12.5
07:01:10.26 +00:00:19.7
07:00:27.53 -00:07:02.3
06:57:52.56 -02:41:35.3
06:52:06.25 -04:01:50.1
06:43:20.66 +02:08:46.4
06:38:00.88 -00:13:22.9
06:40:18.84 -04:30:20.6
07:09:11.08 -05:50:46.7
06:43:14.27 -00:36:30.1
###################################################################################
06:37:31.62 -01:23:42.9 -- not an asteroid (will add it to exclusion list)
07:04:06.78 -01:54:19.1 -- not an asteroid (will add it to exclusion list)
06:40:38.83 -04:53:10.1 -- not an asteroid (will add it to exclusion list)
07:03:24.11 -02:49:51.8 -- not an asteroid (will add it to exclusion list)
06:43:16.47 +00:21:51.2 -- not an asteroid (will add it to exclusion list)
07:03:25.15 -05:00:43.3 -- not an asteroid (will add it to exclusion list)
07:05:06.40 -04:50:36.9 -- not an asteroid (will add it to exclusion list)
06:59:40.46 -00:39:47.2 -- not an asteroid (will add it to exclusion list)
06:58:26.81 +01:51:58.8 -- not an asteroid (will add it to exclusion list)
07:07:06.90 +01:39:59.6 -- not an asteroid (will add it to exclusion list)
07:06:38.32 -03:18:53.8 -- not an asteroid (will add it to exclusion list)
07:01:00.97 -00:25:44.3 -- not an asteroid (will add it to exclusion list)
07:05:18.23 -01:23:01.5 -- not an asteroid (will add it to exclusion list)
07:06:22.88 -01:50:00.4 -- not an asteroid (will add it to exclusion list)
07:05:04.34 -05:27:56.0 -- not an asteroid (will add it to exclusion list)
07:01:07.63 -03:14:32.1 -- not an asteroid (will add it to exclusion list)
07:01:19.13 -03:06:46.0 -- not an asteroid (will add it to exclusion list)
07:01:11.44 -02:08:50.1 -- not an asteroid (will add it to exclusion list)
07:05:51.51 -01:07:33.2 -- not an asteroid (will add it to exclusion list)
07:00:56.86 -03:16:18.5 -- not an asteroid (will add it to exclusion list)
07:07:11.46 -02:58:22.0 -- not an asteroid (will add it to exclusion list)
07:04:39.04 -04:57:05.7 -- not an asteroid (will add it to exclusion list)
07:08:12.65 -03:12:27.9 -- not an asteroid (will add it to exclusion list)
07:06:30.46 -06:00:02.1 -- not an asteroid (will add it to exclusion list)
07:05:14.68 +00:02:13.0 -- not an asteroid (will add it to exclusion list)
07:01:59.65 -03:44:51.2 -- not an asteroid (will add it to exclusion list)
07:05:41.86 -01:12:41.9 -- not an asteroid (will add it to exclusion list)
07:08:03.19 -03:37:55.5 -- not an asteroid (will add it to exclusion list)
07:01:50.92 -01:07:00.2 -- not an asteroid (will add it to exclusion list)
07:08:44.04 -01:45:46.0 -- not an asteroid (will add it to exclusion list)
06:55:49.94 -01:35:05.7 -- not an asteroid (will add it to exclusion list)
06:59:52.95 -04:47:26.6 -- not an asteroid (will add it to exclusion list)
06:56:45.24 +00:46:35.9 -- not an asteroid (will add it to exclusion list)
07:08:03.39 -03:34:27.0 -- not an asteroid (will add it to exclusion list)
06:52:07.78 +00:28:18.4 -- not an asteroid (will add it to exclusion list)
07:03:52.76 -06:00:22.7 -- not an asteroid (will add it to exclusion list)
07:02:31.17 -03:26:38.0 -- not an asteroid (will add it to exclusion list)
07:00:38.94 -02:48:52.4 -- not an asteroid (will add it to exclusion list)
07:01:48.91 +01:06:05.9 -- not an asteroid (will add it to exclusion list)
07:06:12.26 -04:08:44.2 -- not an asteroid (will add it to exclusion list)
06:59:39.95 +01:04:05.3 -- not an asteroid (will add it to exclusion list)
07:03:04.49 -01:18:37.5 -- not an asteroid (will add it to exclusion list)
06:54:15.95 -00:38:33.5 -- not an asteroid (will add it to exclusion list)
06:52:57.35 -03:04:56.8 -- not an asteroid (will add it to exclusion list)
07:07:59.74 -01:46:27.0 -- not an asteroid (will add it to exclusion list)
07:04:54.95 -01:47:05.8 -- not an asteroid (will add it to exclusion list)
06:57:15.16 -02:29:05.7 -- not an asteroid (will add it to exclusion list)
06:44:31.52 +00:07:36.7 -- not an asteroid (will add it to exclusion list)
06:40:17.51 -04:25:58.6 -- not an asteroid (will add it to exclusion list)
06:56:22.08 -00:53:12.5 -- not an asteroid (will add it to exclusion list)
07:01:10.26 +00:00:19.7 -- not an asteroid (will add it to exclusion list)
07:00:27.53 -00:07:02.3 -- not an asteroid (will add it to exclusion list)
06:57:52.56 -02:41:35.3 -- not an asteroid (will add it to exclusion list)
06:52:06.25 -04:01:50.1 -- not an asteroid (will add it to exclusion list)
06:43:20.66 +02:08:46.4 -- not an asteroid (will add it to exclusion list)
06:38:00.88 -00:13:22.9 -- not an asteroid (will add it to exclusion list)
06:40:18.84 -04:30:20.6 -- not an asteroid (will add it to exclusion list)
07:09:11.08 -05:50:46.7 -- not an asteroid (will add it to exclusion list)
06:43:14.27 -00:36:30.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:37:31.62 -01:23:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:00.88 -00:13:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:17.51 -04:25:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:18.84 -04:30:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:38.83 -04:53:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.27 -00:36:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:16.47 +00:21:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:20.66 +02:08:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.52 +00:07:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.25 -04:01:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:07.78 +00:28:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.35 -03:04:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.95 -00:38:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:49.94 -01:35:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.08 -00:53:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.24 +00:46:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:15.16 -02:29:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:52.56 -02:41:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:26.81 +01:51:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:39.95 +01:04:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.46 -00:39:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:52.95 -04:47:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:27.53 -00:07:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:38.94 -02:48:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.86 -03:16:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.97 -00:25:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:07.63 -03:14:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.26 +00:00:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:11.44 -02:08:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.13 -03:06:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:48.91 +01:06:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:50.92 -01:07:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:59.65 -03:44:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:31.17 -03:26:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.49 -01:18:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.11 -02:49:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.15 -05:00:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.76 -06:00:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:06.78 -01:54:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:39.04 -04:57:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:54.95 -01:47:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:04.34 -05:27:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:06.40 -04:50:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.68 +00:02:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.23 -01:23:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.86 -01:12:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:51.51 -01:07:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:12.26 -04:08:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:22.88 -01:50:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:30.46 -06:00:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:38.32 -03:18:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.90 +01:39:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.46 -02:58:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:59.74 -01:46:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:03.19 -03:37:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:03.39 -03:34:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:12.65 -03:12:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.04 -01:45:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:11.08 -05:50:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:37:31.62 -01:23:42.9 -- a known variable star
06:38:00.88 -00:13:22.9 -- a known variable star
06:40:17.51 -04:25:58.6 -- a known variable star
06:40:18.84 -04:30:20.6 -- not a known variable star
06:40:38.83 -04:53:10.1 -- not a known variable star
06:43:14.27 -00:36:30.1 -- a known variable star
06:43:16.47 +00:21:51.2 -- a known variable star
06:43:20.66 +02:08:46.4 -- a known variable star
06:44:31.52 +00:07:36.7 -- not a known variable star
06:52:06.25 -04:01:50.1 -- a known variable star
06:52:07.78 +00:28:18.4 -- not a known variable star
06:52:57.35 -03:04:56.8 -- not a known variable star
06:54:15.95 -00:38:33.5 -- not a known variable star
06:55:49.94 -01:35:05.7 -- not a known variable star
06:56:22.08 -00:53:12.5 -- a known variable star
06:56:45.24 +00:46:35.9 -- not a known variable star
06:57:15.16 -02:29:05.7 -- not a known variable star
06:57:52.56 -02:41:35.3 -- not a known variable star
06:58:26.81 +01:51:58.8 -- not a known variable star
06:59:39.95 +01:04:05.3 -- a known variable star
06:59:40.46 -00:39:47.2 -- not a known variable star
06:59:52.95 -04:47:26.6 -- not a known variable star
07:00:27.53 -00:07:02.3 -- not a known variable star
07:00:38.94 -02:48:52.4 -- a known variable star
07:00:56.86 -03:16:18.5 -- not a known variable star
07:01:00.97 -00:25:44.3 -- not a known variable star
07:01:07.63 -03:14:32.1 -- a known variable star
07:01:10.26 +00:00:19.7 -- a known variable star
07:01:11.44 -02:08:50.1 -- not a known variable star
07:01:19.13 -03:06:46.0 -- not a known variable star
07:01:48.91 +01:06:05.9 -- not a known variable star
07:01:50.92 -01:07:00.2 -- not a known variable star
07:01:59.65 -03:44:51.2 -- not a known variable star
07:02:31.17 -03:26:38.0 -- not a known variable star
07:03:04.49 -01:18:37.5 -- not a known variable star
07:03:24.11 -02:49:51.8 -- not a known variable star
07:03:25.15 -05:00:43.3 -- a known variable star
07:03:52.76 -06:00:22.7 -- not a known variable star
07:04:06.78 -01:54:19.1 -- not a known variable star
07:04:39.04 -04:57:05.7 -- not a known variable star
07:04:54.95 -01:47:05.8 -- not a known variable star
07:05:04.34 -05:27:56.0 -- not a known variable star
07:05:06.40 -04:50:36.9 -- a known variable star
07:05:14.68 +00:02:13.0 -- not a known variable star
07:05:18.23 -01:23:01.5 -- a known variable star
07:05:41.86 -01:12:41.9 -- not a known variable star
07:05:51.51 -01:07:33.2 -- not a known variable star
07:06:12.26 -04:08:44.2 -- a known variable star
07:06:22.88 -01:50:00.4 -- not a known variable star
07:06:30.46 -06:00:02.1 -- a known variable star
07:06:38.32 -03:18:53.8 -- a known variable star
07:07:06.90 +01:39:59.6 -- not a known variable star
07:07:11.46 -02:58:22.0 -- not a known variable star
07:07:59.74 -01:46:27.0 -- not a known variable star
07:08:03.19 -03:37:55.5 -- a known variable star
07:08:03.39 -03:34:27.0 -- a known variable star
07:08:12.65 -03:12:27.9 -- not a known variable star
07:08:44.04 -01:45:46.0 -- not a known variable star
07:09:11.08 -05:50:46.7 -- a known variable star
Found 38 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
59 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 59 (excluding asteroids and hot pixels, 38 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)2461144.60625929 -observatory V36
23:57:26.48 -03:04:05.5 Mercury (0.1mag)
02:59:24.67 +17:08:06.5 Venus (-3.9mag)
00:12:27.56 +00:16:21.0 Mars (1.2mag)
07:11:47.35 +22:47:36.4 Jupiter (-2.1mag)
00:28:20.12 +00:43:42.2 Saturn (0.9mag)
03:47:18.07 +19:46:12.4 Uranus (5.8mag)
00:10:35.49 -00:16:56.4 Neptune (7.8mag)
20:33:40.10 -22:52:31.4 Pluto (14.5mag)
22:42:05.27 -08:20:20.1 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 13 21:37 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.60625929:
07:11:42.35 +22:47:48.5 Io (5.8mag)
07:11:47.48 +22:47:33.0 Europa (5.9mag)
07:11:54.82 +22:47:27.7 Ganymede (5.3mag)
07:12:13.10 +22:46:51.0 Callisto (6.6mag)
07:15:12.49 +22:36:07.4 Himalia (15.3mag)
07:11:45.07 +22:47:39.3 Thebe (16.2mag)
07:15:21.40 +23:06:09.7 Elara (17.3mag)
07:10:32.50 +23:28:36.2 Pasiphae (17.4mag)
07:20:09.55 +22:45:26.4 Carme (18.5mag)
00:28:28.32 +00:43:57.9 Titan (8.8mag)
00:28:22.64 +00:43:55.4 Rhea (10.1mag)
00:28:03.56 +00:44:09.7 Iapetus (11.5mag)
00:28:33.54 +00:43:50.7 Hyperion (14.8mag)
00:29:58.51 +00:52:42.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 21:37 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.60625929:
15:29:51.37 -14:52:16.3 JWST
16:53:39.49 +44:54:50.6 Chandra
07:49:56.75 -32:48:47.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 21:37 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.60625929 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:12.30 -28:40:07.1 13.9mag P/2010 H2 (Vales)
05:05:23.13 -69:45:07.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:02.59 +31:25:28.8 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.59 +10:19:22.5 17.6mag C/2021 G2 (ATLAS)
23:09:42.79 +29:09:16.0 17.1mag C/2022 E2 (ATLAS)
04:27:02.01 +25:59:13.0 16.0mag C/2022 N2 (PANSTARRS)
09:03:01.71 +32:00:18.9 16.2mag C/2022 QE78 (ATLAS)
08:30:47.58 -00:21:16.6 17.3mag C/2022 R6 (PANSTARRS)
18:54:10.14 +18:22:23.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:16.80 -11:32:57.3 17.5mag P/2023 B1 (PANSTARRS)
09:08:31.74 -12:11:15.7 17.6mag C/2023 F3 (ATLAS)
21:52:17.44 +62:47:46.7 17.5mag C/2023 H5 (Lemmon)
19:20:48.14 -03:42:08.4 14.2mag C/2023 R1 (PANSTARRS)
21:35:59.23 +85:38:59.7 17.8mag C/2023 X2 (Lemmon)
06:17:02.66 +63:31:19.9 17.1mag C/2024 A1 (ATLAS)
05:09:11.07 +17:39:57.7 10.9mag C/2024 E1 (Wierzchos)
16:20:28.98 +06:04:47.7 17.4mag C/2024 G6 (ATLAS)
20:20:16.10 +14:45:42.1 14.6mag C/2024 J3 (ATLAS)
03:24:40.31 -22:40:29.4 16.4mag C/2024 T5 (ATLAS)
05:15:06.72 +45:45:49.7 17.7mag C/2025 J1 (Borisov)
13:46:42.60 +44:12:29.2 15.1mag C/2025 L1 (ATLAS)
03:22:17.70 -25:55:04.4 17.8mag C/2025 Q3 (ATLAS)
23:28:18.01 +19:09:26.7 8.8mag C/2025 R3 (PANSTARRS)
12:54:56.43 +02:53:49.5 17.4mag C/2025 Y1 (ATLAS)
03:11:34.75 +02:50:35.5 12.7mag C/2026 A1 (MAPS)
23:54:11.08 +36:52:00.9 14.5mag C/2026 B2 (Sun-Gao)
18:39:14.82 -09:49:12.3 11.9mag 10P/Tempel
15:02:51.86 +03:24:12.8 13.8mag 24P/Schaumasse
11:03:19.03 -01:35:15.5 15.7mag 29P/Schwassmann-Wachmann
18:00:22.96 -09:40:49.0 17.9mag 40P/Vaisala
10:37:39.92 -04:15:03.5 16.9mag 43P/Wolf-Harrington
01:45:44.50 +17:09:52.4 17.2mag 47P/Ashbrook-Jackson
07:07:16.96 +37:25:09.2 17.0mag 63P/Wild
23:26:38.16 -11:40:43.9 15.7mag 65P/Gunn
03:58:12.04 +20:36:04.1 15.9mag 76P/West-Kohoutek-Ikemura
01:01:23.37 +07:51:22.5 14.3mag 78P/Gehrels
22:57:15.01 -09:57:04.0 14.6mag 88P/Howell
02:05:02.96 +20:08:09.2 15.1mag 93P/Lovas
04:51:14.70 +32:11:10.6 16.2mag 123P/West-Hartley
08:26:09.48 +39:14:07.1 16.2mag 124P/Mrkos
02:30:17.43 +14:09:30.5 16.4mag 128P/Shoemaker-Holt
02:43:49.33 +14:15:41.2 17.5mag 131P/Mueller
01:16:14.17 +12:34:41.5 10.7mag 141P/Machholz
01:25:25.45 +04:09:46.1 10.7mag 141P-A/Machholz
00:11:38.48 +00:08:36.6 13.0mag 141P-D/Machholz
01:55:35.25 +05:54:55.5 17.8mag 141P-I/Machholz
00:57:05.76 -02:28:41.0 15.1mag 162P/SidingSpring
10:29:06.69 +30:57:45.2 18.0mag 164P/Christensen
06:33:01.74 +24:18:06.3 18.0mag 198P/ODAS
14:54:48.16 -00:15:57.9 17.6mag 210P/Christensen
21:33:19.90 -11:54:19.2 17.6mag 218P/LINEAR
17:16:03.49 -14:09:36.4 16.1mag 235P/LINEAR
05:30:23.85 +34:33:12.7 16.7mag 240P/NEAT
07:37:34.41 -05:22:24.2 17.7mag 242P/Spahr
22:12:10.41 -21:28:50.3 17.9mag 260P/McNaught
15:43:22.37 +06:51:53.5 17.5mag 391P/Kowalski
07:33:28.72 +21:21:35.1 17.7mag 450P/LONEOS
05:33:06.85 +45:08:37.5 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 21:37 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 21:37 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 21:37 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
10:01:10.740 +29:37:27.72 AT 2026iuk 2026-04-05.76 21.01
11:10:23.800 +30:53:36.06 AT 2026iuj 2026-04-04.83 20.45
11:10:19.760 +34:35:07.49 AT 2026iui 2026-04-04.79 21
11:03:07.270 +39:55:31.99 AT 2026iuh 2026-04-04.78 20.75
-rw-r--r-- 1 apache apache 30K Apr 13 21:37 tns_transients_list.txt
