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_213659_TTUQ2b1x1_24742_7XdClvXM
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,2461144.6077,10.34,0.05,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
SY Mon 20260414.1077 10.34CV 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,2461144.6077,12.94,0.05,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 20260414.1077 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8499-02.8303,2461144.6077,12.70,0.05,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 20260414.1077 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.55,0.05,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
target 20260414.1077 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0896-02.7869,2461144.6077,12.74,0.05,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 J107.0896-02.7869 20260414.1077 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0658496-010628,2461144.6077,12.39,0.05,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
GDS_J0658496-010628 20260414.1077 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 J105.5594-03.0943,2461144.6077,12.59,0.05,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 J105.5594-03.0943 20260414.1077 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 3119455362927855488,2461144.6077,12.12,0.05,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 3119455362927855488 20260414.1077 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108620917091030272,2461144.6077,12.42,0.05,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
Gaia DR3 3108620917091030272 20260414.1077 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 3109471389332247552,2461144.6077,12.32,0.05,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 3109471389332247552 20260414.1077 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
Gaia DR3 3105548121386329600,2461144.6077,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105548121386329600 20260414.1077 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112750781541980032,2461144.6077,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112750781541980032 20260414.1077 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112693400776779776,2461144.6077,11.97,0.05,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 3112693400776779776 20260414.1077 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1626-04.9704,2461144.6077,12.04,0.05,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 20260414.1077 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3280-03.1171,2461144.6077,11.97,0.05,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 20260414.1077 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101373967233337984,2461144.6077,12.11,0.05,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
Gaia DR3 3101373967233337984 20260414.1077 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.07,0.05,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 20260414.1077 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107988968482458496,2461144.6077,12.27,0.05,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
Gaia DR3 3107988968482458496 20260414.1077 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
ATO J106.9785-02.1149,2461144.6077,12.28,0.05,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
ATO J106.9785-02.1149 20260414.1077 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
target,2461144.6077,12.23,0.05,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
target 20260414.1077 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
ATO J106.4234-01.2112,2461144.6077,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4234-01.2112 20260414.1077 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1077 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1845-01.7588,2461144.6077,12.40,0.05,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 J107.1845-01.7588 20260414.1077 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 3112749274012032640,2461144.6077,12.52,0.05,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 20260414.1077 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112882349279538816,2461144.6077,12.54,0.05,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 3112882349279538816 20260414.1077 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 J104.1953-03.4629,2461144.6077,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.1953-03.4629 20260414.1077 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101628912187905408,2461144.6077,12.27,0.05,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
Gaia DR3 3101628912187905408 20260414.1077 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
ATO J106.2256-01.7850,2461144.6077,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2256-01.7850 20260414.1077 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.6319-03.4457,2461144.6077,12.40,0.05,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 J105.6319-03.4457 20260414.1077 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
target,2461144.6077,12.55,0.05,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
target 20260414.1077 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 3114653353273377664,2461144.6077,12.54,0.05,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 3114653353273377664 20260414.1077 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 J103.4899-04.8802,2461144.6077,12.40,0.05,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 J103.4899-04.8802 20260414.1077 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
target,2461144.6077,12.28,0.05,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
target 20260414.1077 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 J106.4248-01.4982,2461144.6077,12.54,0.05,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
ATO J106.4248-01.4982 20260414.1077 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 J105.5007-03.7484,2461144.6077,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5007-03.7484 20260414.1077 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.72,0.05,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 20260414.1077 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1077 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070804.67-033414.7,2461144.6077,12.59,0.05,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
ZTF J070804.67-033414.7 20260414.1077 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,2461144.6077,12.74,0.05,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 20260414.1077 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461144.6077,12.52,0.05,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 20260414.1077 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112649905648673536,2461144.6077,12.64,0.05,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 3112649905648673536 20260414.1077 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1077 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102665240558896256,2461144.6077,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102665240558896256 20260414.1077 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.62,0.05,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
target 20260414.1077 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1077 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5085-01.9908,2461144.6077,12.92,0.05,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 J103.5085-01.9908 20260414.1077 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112223290836561024,2461144.6077,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112223290836561024 20260414.1077 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6077,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1077 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9279-01.2566,2461144.6077,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9279-01.2566 20260414.1077 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J064217.78+005441.1,2461144.6077,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064217.78+005441.1 20260414.1077 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
2MASS J06552398-0526278,2461144.6077,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J06552398-0526278 20260414.1077 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
V0918 Mon,2461144.6077,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0918 Mon 20260414.1077 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J0634409-033733,2461144.6077,12.34,0.05,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
NSVS J0634409-033733 20260414.1077 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
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+020852,2461144.6077,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0643204+020852 20260414.1077 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
V0785 Mon,2461144.6077,10.79,0.05,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
V0785 Mon 20260414.1077 10.79CV 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
Date (UTC)
JD(UTC)
mag.
R.A. & Dec.(J2000)
X & Y (pix)
Image
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
ZTF J063934.65-040636.1,2461144.6077,12.09,0.05,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
ZTF J063934.65-040636.1 20260414.1077 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
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,2461144.6077,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Mon 20260414.1077 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 12529703,2461144.6077,11.39,0.05,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
NSVS 12529703 20260414.1077 11.39CV 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
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,2461144.6077,9.40,0.05,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 20260414.1077 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 J0643141-003633,2461144.6077,12.21,0.05,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
NSVS J0643141-003633 20260414.1077 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
## 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: 2461144.60802894 14.04.2026 02:35:23.700 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 28910
Objects passed selection criteria: 28764
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: 20794.8
Average stars matched: 19023 (91.4798 %)
Memory usage VmPeak: 131296 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 21:43:30 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: 2461144.60802894 14.04.2026 02:35:23.700 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 215
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: 93 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): 212012
Objects passed selection criteria: 211340
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: 151996
Average stars matched: 138472 (91.1024 %)
Memory usage VmPeak: 1955564 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 21:50:04 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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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: 2461144.60745134
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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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 06:51:28.965 -01:59:54.75
Angular distance between the image centers 0.0591 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 06:51:28.876 -01:59:48.31
Angular distance between the image centers 0.0597 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 06:51:28.965 -01:59:54.75
Second-epoch second image center 06:51:28.876 -01:59:48.31
Angular distance between the image centers 0.00183 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.Hf4cI2EQpi
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.CcaKZOnCcZ
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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits &> /tmp/tmp.xHK3zvmQiR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits &> /tmp/tmp.xGSd5PWlzQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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 5 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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
All-image limiting magnitude estimate: 14.0 (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.Hf4cI2EQpi (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_213659_TTUQ2b1x1_24742_7XdClvXM/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.CcaKZOnCcZ (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_213659_TTUQ2b1x1_24742_7XdClvXM/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.xHK3zvmQiR (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_213659_TTUQ2b1x1_24742_7XdClvXM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1330, passed=17210
Got 17210 stars (including 15866 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat
util/solve_plate_with_UCAC5 got 17210 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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 16770 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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 16773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 16773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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.xGSd5PWlzQ (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_213659_TTUQ2b1x1_24742_7XdClvXM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1363, passed=17353
Got 17353 stars (including 15974 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat
util/solve_plate_with_UCAC5 got 17353 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(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 16955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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: 928 matched stars entering correct_measured_positions(), 16955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 16955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 928 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_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/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_213659_TTUQ2b1x1_24742_7XdClvXM/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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21092.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 53757_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 53757_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:13.69 -02:21:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21092_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 21092_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06678_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 06678_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:35:46.88 -05:22:33.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51629_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 51629_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:56.43 -00:17:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 0.864 3111213290627286400 107.23536505496 -00.29008246977 11.1544 9.7065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21644_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 21644_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:33:38.29 -01:13:13.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
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 ####
06:37:31.61 -01:23:43.5
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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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 06:51:28.965 -01:59:54.75
Angular distance between the image centers 0.0591 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 06:51:28.876 -01:59:48.31
Angular distance between the image centers 0.0597 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 06:51:28.965 -01:59:54.75
Second-epoch second image center 06:51:28.876 -01:59:48.31
Angular distance between the image centers 0.00183 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.DnEY0cYp1t
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.b4DUDHqUXN
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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits &> /tmp/tmp.Caqhb5SqpA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits &> /tmp/tmp.T6Ck1480IJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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 184 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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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.DnEY0cYp1t (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_213659_TTUQ2b1x1_24742_7XdClvXM/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.b4DUDHqUXN (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_213659_TTUQ2b1x1_24742_7XdClvXM/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.Caqhb5SqpA (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_213659_TTUQ2b1x1_24742_7XdClvXM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=13628, passed=114667
Got 114667 stars (including 100938 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat
util/solve_plate_with_UCAC5 got 114667 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: 925 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 111311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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(), 111310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 111331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 926 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.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.T6Ck1480IJ (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_213659_TTUQ2b1x1_24742_7XdClvXM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q2b1x1_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=13793, passed=114384
Got 114384 stars (including 100484 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat
util/solve_plate_with_UCAC5 got 114384 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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 110623 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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 110621 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 110643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 928 stars left (next iteration limit 1019)
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_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/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_213659_TTUQ2b1x1_24742_7XdClvXM/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_21-34-33_20.00sec_-5.00C_LIGHT_0644.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_213659_TTUQ2b1x1_24742_7XdClvXM/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-34-33_20.00sec_-5.00C_LIGHT_0644.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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_213659_TTUQ2b1x1_24742_7XdClvXM/wcs_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645.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__out270183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out306284.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out122793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out220085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out221821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90090.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 76s
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: 36s
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Considering the candidate 283493_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283493_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:03:27.53 -02:23:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.080 3108835150058693120 105.86429971813 -02.38943656729 14.0290 13.4552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283499_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283499_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283501_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283501_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:20.02 -01:07:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.916 3112179314673468544 105.33422604982 -01.12977167403 13.7526 13.2200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283507_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283507_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:52.40 -00:44:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.895 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283514_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283514_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283515_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283515_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283521_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283521_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283522_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283522_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:20.76 -00:46:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.605 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283530_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283530_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283531_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283531_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283536_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283536_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:03.98 -00:02:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.085 3112734769903489536 106.51609385568 -00.03830975549 13.4506 12.6183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283538_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283538_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283541_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283541_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283544_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283544_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:53:54.06 +01:48:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.895 3114192550524702208 103.47481321244 +01.81526900993 13.1717 12.7564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283549_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283549_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283554_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283554_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283562_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283562_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283563_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:31.71 +02:11:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283566_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283566_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:51:02.48 +01:07:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283568_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283568_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:52:13.37 -00:19:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283569_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283569_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:54:08.21 -05:53:04.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 283570_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283570_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:36.76 -01:40:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283572_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283572_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:13.82 -03:36:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283573_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 283573_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 283574_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283574_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:05:51.03 -02:39:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.470 3108763162105399680 106.46205315191 -02.66360225252 12.0388 11.0733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283575_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283575_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:18.41 -01:42:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.842 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283580_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283580_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:37.17 -05:34:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 1.098 3053328019221116672 106.90468109872 -05.56898615361 12.2211 11.3918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283582_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283582_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:51:45.62 +00:30:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283583_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283583_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:26.99 -01:50:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.600 3109207296085297536 106.86238560713 -01.84331649968 12.1404 11.6766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283587_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 283587_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:49.52 -05:43:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 286419_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 286419_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 287047_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 287047_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 287757_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 287757_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 288760_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 288760_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:05:27.38 -03:20:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 4.467 3107881255000913152 106.36288380293 -03.34481404916 11.7246 10.8001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290162_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 290162_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:51:39.66 +00:25:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290792_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 290792_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:40:30.68 -01:04:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291477_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 291477_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:10.69 -03:14:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291677_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 291677_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 292088_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 292088_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:38.01 -05:29:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292851_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 292851_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:02:11.30 -06:02:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294540_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 294540_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:50:41.65 -00:33:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294708_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 294708_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:16.57 -04:03:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295468_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 295468_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:05:52.43 -01:02:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295891_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 295891_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:52:25.49 -05:17:26.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 297417_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 297417_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:10.50 +00:02:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.709 3112774390980328320 106.04409922559 +00.04009490383 12.8697 12.0978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298069_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 298069_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:59:35.86 +00:49:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 4.345 3113827242086041984 104.89999945513 +00.83322365418 12.8202 11.8115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298457_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 298457_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:52.74 -01:19:04.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298582_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 298582_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:14.46 -03:20:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.166 3107916435071192576 107.05938152547 -03.33918560888 12.7734 12.0959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298915_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 298915_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:36:40.94 -05:13:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 299466_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 299466_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 299640_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 299640_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 299647_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 299647_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:02:39.75 -04:37:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299748_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 299748_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:18.45 -03:02:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.810 3108655929664211072 106.07666031661 -03.03495984401 13.0643 12.6085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 299755_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 299755_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:53:08.20 -04:35:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300232_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 300232_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 300294_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 300294_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:00:06.63 -02:51:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300474_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 300474_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 300627_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 300627_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:00:50.41 -04:30:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.552 3101735908414140416 105.20979162595 -04.51016365204 12.8843 12.0606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300832_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 300832_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:52.49 -00:27:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 301088_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301088_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:02:22.99 +00:25:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.773 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301183_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301183_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:03:41.84 -00:34:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 5.691 3112600358906822784 105.92435322766 -00.57610862188 12.3354 11.1129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301206_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301206_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:17.27 +00:25:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.791 3114280099135354112 107.07174264372 +00.43204080684 12.8009 11.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301242_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301242_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 301272_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301272_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 301490_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301490_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:00:21.35 -05:50:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.644 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301536_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301536_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:32.30 -05:17:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.790 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301550_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 301550_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 301759_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 301759_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:54:30.15 -04:07:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 301976_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 301976_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 302270_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 302270_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 302388_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 302388_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:00:51.59 -03:52:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.490 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302611_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 302611_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:54:09.45 -05:52:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 302678_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 302678_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:37.59 -01:22:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.001 3109339379218885888 107.40665275024 -01.37683283674 13.0624 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302931_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 302931_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:43.65 -00:29:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.895 3112692889681609088 106.18162536672 -00.49277504927 13.1660 12.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302973_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 302973_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:22.91 -04:08:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.177 3107533946769387392 107.34498467445 -04.14990516113 12.9877 12.2399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303087_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 303087_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 303471_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 303471_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:44.70 -00:27:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.540 3112693125898976128 106.18617333971 -00.46329564351 13.2235 12.3843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303909_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 303909_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:51.38 -01:46:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.880 3109234234118285952 107.21394667394 -01.77617496224 13.0380 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304104_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 304104_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:50:44.44 -00:31:38.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 304110_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 304110_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:30.45 -06:00:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304186_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 304186_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 304214_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 304214_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 304338_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 304338_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 304409_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 304409_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 304655_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 304655_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:37:58.69 -01:25:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305286_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305286_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:02:47.47 -04:14:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 305406_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305406_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:05:28.02 +01:29:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 5.354 3114638612946094336 106.36647147059 +01.49234473238 13.4661 12.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305587_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305587_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:23.67 +00:30:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.341 3114292571720574464 107.09853168373 +00.50913942528 13.2073 12.2839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305639_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 305639_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 305752_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305752_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:56:27.58 +00:06:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.248 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305795_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305795_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:51:28.89 -00:00:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305796_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 305796_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 305919_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 305919_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:56:45.72 +00:46:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306026_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 306026_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 306144_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306144_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:03.43 -02:29:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.883 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306225_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306225_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:58.68 -00:56:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.680 3109605186152914432 106.99387176228 -00.94487186150 13.3450 12.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306284_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306284_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:59:02.55 -03:29:52.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 306285_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306285_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 306412_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306412_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:47:26.35 +02:03:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.355 3126362769851744256 101.85924991798 +02.06333923017 13.2439 12.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306418_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306418_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:58:39.01 -04:20:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.183 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306609_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306609_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:22.47 -03:06:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306682_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306682_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:08.57 -03:35:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.766 3107717565213010816 107.03467099261 -03.58332209027 13.3745 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306906_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 306906_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:45:00.24 -00:03:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306943_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 306943_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 306960_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 306960_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307010_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307010_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307059_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307059_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307135_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 307135_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:03:39.60 -00:16:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.768 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307167_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307167_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307212_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307212_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307274_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 307274_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:03:08.05 -03:16:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.417 3108621599983160704 105.78322570098 -03.27201335860 13.1919 12.4770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307794_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307794_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307811_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 307811_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 307883_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 307883_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:01:51.04 -01:07:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.167 3112551568078572160 105.46258255986 -01.11679803352 13.3869 13.0466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308006_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 308006_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:43:50.19 +01:35:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308103_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 308103_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:07:12.78 -04:08:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.039 3107567000838631936 106.80293572744 -04.13605509089 13.4970 13.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308412_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 308412_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 308562_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 308562_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:59:40.09 +01:04:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.567 3113869985600410112 104.91674694958 +01.06740623641 13.5646 13.3346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308632_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 308632_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 308666_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 308666_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308952_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 308952_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:34.89 -05:56:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309063_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 309063_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:21.11 +01:30:23.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 309204_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 309204_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 309242_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 309242_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 309381_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 309381_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:39.99 -05:47:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309453_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 309453_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:38:54.27 +00:00:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.728 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309464_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 309464_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:45:04.87 -01:02:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.876 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309538_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 309538_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 309695_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 309695_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:53:07.51 -01:52:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309860_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 309860_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 310037_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310037_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:37.19 -04:38:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.358 3101496459701712640 106.65476195883 -04.63532880131 13.6813 13.0848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310273_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310273_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:54:23.41 -01:37:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.272 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310346_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310346_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:48:13.71 -01:19:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 310409_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310409_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:48:48.54 +00:23:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.615 3113610294697190784 102.20183118370 +00.39122776001 13.6085 13.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310563_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310563_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 310585_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 310585_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 310617_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310617_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:51.42 -02:16:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.426 3108857002851931776 106.21398983457 -02.28187184212 13.3926 12.6907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310907_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 310907_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:11.91 +00:18:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.096 3114262610029958784 106.54920449104 +00.30906939611 13.7638 13.2801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311612_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 311612_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:06:29.81 -05:59:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311652_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 311652_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 312488_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 312488_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 312715_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 312715_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 313140_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 313140_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:37:19.43 +00:16:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 5.447 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313184_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 313184_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 313608_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 313608_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 313655_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 313655_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 313918_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 313918_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:04:05.06 -02:22:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.424 3108833221613004800 106.02064200889 -02.37978674497 13.9010 13.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314330_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 314330_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:59:57.31 -00:05:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.709 3112885196837878016 104.98858288935 -00.08675063744 13.5793 12.7573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315275_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 315275_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 315368_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 315368_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 237671_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 237671_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:40:09.04 +01:22:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.711 3126632974834859392 100.03692742394 +01.37171623584 12.6357 11.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248954_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 248954_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 43125_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 43125_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:09:13.68 -02:21:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 07:08:45.31 +00:41:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122793_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 122793_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 47993_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 47993_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:51:26.31 -05:15:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 47889_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:44:47.62 -05:17:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90090_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 90090_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 221821_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 221821_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 270183_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 270183_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:36:36.45 -01:48:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.735 3106779956665024640 099.15114398779 -01.80856584193 12.3593 10.7523 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 176200_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 176200_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 57802_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 57802_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:45:42.45 -04:56:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152309_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 152309_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:37:31.61 -01:23:42.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:41:59.39 -01:11:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267725_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 267725_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:37:53.43 -05:55:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31629_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 31629_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 158645_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 158645_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:55:00.57 -01:02:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220085_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 220085_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:50:00.75 +01:46:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80449_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 80449_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 265915_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 265915_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:52:00.41 +00:12:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.988 3113357819339125504 103.00115885910 +00.20192758615 11.7103 10.0166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 49190_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 49190_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 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_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 127999_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:49:16.35 -02:16:18.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154375_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 154375_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:48:19.08 -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_21-35-23_20.00sec_-4.90C_LIGHT_0645
Preparing report for the candidate 169635_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
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Considering the candidate 173456_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 173456_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:50:49.77 -00:32:34.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121814_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 121814_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 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_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 107626_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:34:21.74 -03:04:27.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 198847_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 198847_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:41:05.51 +00:29:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 157311_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 157311_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:33:38.21 -01:13:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53553_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 53553_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:36:35.42 -05:12:39.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247718_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645
The candidate 247718_fd_Mon-02-Q2b1x1_2026-04-13_21-35-23_20.00sec_-4.90C_LIGHT_0645 did not pass the final checks
**** FOUND 06:35:16.03 +00:53:22.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 115s
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 ####
06:37:31.61 -01:23:43.5
06:55:40.26 -02:20:14.6
06:43:14.11 -00:36:30.4
07:08:56.42 -00:17:23.4
06:50:17.84 +02:13:22.6
06:43:20.67 +02:08:46.3
06:42:18.02 +00:54:40.1
06:39:35.03 -04:06:33.0
07:02:23.53 -01:34:45.2
07:03:24.15 -02:49:51.6
06:46:14.00 +00:50:46.5
07:08:21.63 -02:47:09.9
06:58:49.24 -01:06:26.0
07:02:14.55 -03:05:58.7
06:43:00.33 -00:24:45.9
07:02:50.48 -03:19:42.3
07:05:18.16 -01:23:00.4
06:42:09.91 -03:38:13.0
07:05:15.70 +00:02:29.9
07:05:10.39 -00:29:31.3
07:04:39.00 -04:57:05.9
07:01:19.09 -03:06:46.3
07:01:27.45 -05:22:48.4
07:00:56.84 -03:16:18.6
07:07:11.54 -02:58:22.4
07:07:54.74 -02:07:28.1
06:56:45.17 +00:46:32.9
07:05:41.76 -01:12:42.3
07:01:22.90 -06:08:19.4
07:08:44.07 -01:45:46.1
07:05:14.74 +00:02:12.6
07:01:10.30 +00:00:18.0
06:56:48.11 -03:27:50.6
06:59:52.95 -04:47:25.5
07:04:54.90 -01:47:04.7
07:02:30.71 -03:26:38.2
07:01:48.85 +01:06:04.8
07:04:55.92 +01:34:26.5
06:53:58.15 -04:52:50.3
06:44:31.51 +00:07:32.9
07:05:41.64 -01:30:01.5
07:01:59.75 -03:44:51.5
07:01:10.33 -01:01:15.8
06:54:15.84 -00:38:31.5
07:08:03.40 -03:34:26.0
07:07:00.65 -00:52:23.6
06:56:22.00 -00:53:11.7
07:01:00.38 -00:27:55.6
07:08:06.64 -05:59:32.1
06:59:02.37 -03:28:54.2
06:48:30.59 +00:57:43.9
07:04:33.71 -04:28:39.1
06:53:59.56 -01:59:29.4
06:57:09.52 -01:07:39.0
07:03:33.70 -02:51:42.1
06:59:44.18 -01:15:44.7
07:09:11.07 -05:50:46.2
06:55:24.16 -05:26:25.2
06:52:06.23 -04:01:50.1
06:34:41.23 -03:37:25.5
########### 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 ####
06:37:31.61 -01:23:43.5
07:02:23.53 -01:34:45.2
07:03:24.15 -02:49:51.6
06:46:14.00 +00:50:46.5
07:08:21.63 -02:47:09.9
06:58:49.24 -01:06:26.0
07:02:14.55 -03:05:58.7
06:43:00.33 -00:24:45.9
07:02:50.48 -03:19:42.3
07:05:18.16 -01:23:00.4
06:42:09.91 -03:38:13.0
07:05:15.70 +00:02:29.9
07:05:10.39 -00:29:31.3
07:04:39.00 -04:57:05.9
07:01:19.09 -03:06:46.3
07:01:27.45 -05:22:48.4
07:00:56.84 -03:16:18.6
07:07:11.54 -02:58:22.4
07:07:54.74 -02:07:28.1
06:56:45.17 +00:46:32.9
07:05:41.76 -01:12:42.3
07:01:22.90 -06:08:19.4
07:08:44.07 -01:45:46.1
07:05:14.74 +00:02:12.6
07:01:10.30 +00:00:18.0
06:56:48.11 -03:27:50.6
06:59:52.95 -04:47:25.5
07:04:54.90 -01:47:04.7
07:02:30.71 -03:26:38.2
07:01:48.85 +01:06:04.8
07:04:55.92 +01:34:26.5
06:53:58.15 -04:52:50.3
06:44:31.51 +00:07:32.9
07:05:41.64 -01:30:01.5
07:01:59.75 -03:44:51.5
07:01:10.33 -01:01:15.8
06:54:15.84 -00:38:31.5
07:08:03.40 -03:34:26.0
07:07:00.65 -00:52:23.6
06:56:22.00 -00:53:11.7
07:01:00.38 -00:27:55.6
07:08:06.64 -05:59:32.1
06:59:02.37 -03:28:54.2
06:48:30.59 +00:57:43.9
07:04:33.71 -04:28:39.1
06:53:59.56 -01:59:29.4
06:57:09.52 -01:07:39.0
07:03:33.70 -02:51:42.1
06:59:44.18 -01:15:44.7
06:42:18.02 +00:54:40.1
06:55:24.16 -05:26:25.2
06:55:40.26 -02:20:14.6
06:34:41.23 -03:37:25.5
06:43:20.67 +02:08:46.3
07:08:56.42 -00:17:23.4
06:39:35.03 -04:06:33.0
07:09:11.07 -05:50:46.2
06:50:17.84 +02:13:22.6
06:52:06.23 -04:01:50.1
06:43:14.11 -00:36:30.4
###################################################################################
06:37:31.61 -01:23:43.5 -- not an asteroid (will add it to exclusion list)
07:02:23.53 -01:34:45.2 -- not an asteroid (will add it to exclusion list)
07:03:24.15 -02:49:51.6 -- not an asteroid (will add it to exclusion list)
06:46:14.00 +00:50:46.5 -- not an asteroid (will add it to exclusion list)
07:08:21.63 -02:47:09.9 -- not an asteroid (will add it to exclusion list)
06:58:49.24 -01:06:26.0 -- not an asteroid (will add it to exclusion list)
07:02:14.55 -03:05:58.7 -- not an asteroid (will add it to exclusion list)
06:43:00.33 -00:24:45.9 -- not an asteroid (will add it to exclusion list)
07:02:50.48 -03:19:42.3 -- not an asteroid (will add it to exclusion list)
07:05:18.16 -01:23:00.4 -- not an asteroid (will add it to exclusion list)
06:42:09.91 -03:38:13.0 -- not an asteroid (will add it to exclusion list)
07:05:15.70 +00:02:29.9 -- not an asteroid (will add it to exclusion list)
07:05:10.39 -00:29:31.3 -- not an asteroid (will add it to exclusion list)
07:04:39.00 -04:57:05.9 -- not an asteroid (will add it to exclusion list)
07:01:19.09 -03:06:46.3 -- not an asteroid (will add it to exclusion list)
07:01:27.45 -05:22:48.4 -- not an asteroid (will add it to exclusion list)
07:00:56.84 -03:16:18.6 -- not an asteroid (will add it to exclusion list)
07:07:11.54 -02:58:22.4 -- not an asteroid (will add it to exclusion list)
07:07:54.74 -02:07:28.1 -- not an asteroid (will add it to exclusion list)
06:56:45.17 +00:46:32.9 -- not an asteroid (will add it to exclusion list)
07:05:41.76 -01:12:42.3 -- not an asteroid (will add it to exclusion list)
07:01:22.90 -06:08:19.4 -- not an asteroid (will add it to exclusion list)
07:08:44.07 -01:45:46.1 -- not an asteroid (will add it to exclusion list)
07:05:14.74 +00:02:12.6 -- not an asteroid (will add it to exclusion list)
07:01:10.30 +00:00:18.0 -- not an asteroid (will add it to exclusion list)
06:56:48.11 -03:27:50.6 -- not an asteroid (will add it to exclusion list)
06:59:52.95 -04:47:25.5 -- not an asteroid (will add it to exclusion list)
07:04:54.90 -01:47:04.7 -- not an asteroid (will add it to exclusion list)
07:02:30.71 -03:26:38.2 -- not an asteroid (will add it to exclusion list)
07:01:48.85 +01:06:04.8 -- not an asteroid (will add it to exclusion list)
07:04:55.92 +01:34:26.5 -- not an asteroid (will add it to exclusion list)
06:53:58.15 -04:52:50.3 -- not an asteroid (will add it to exclusion list)
06:44:31.51 +00:07:32.9 -- not an asteroid (will add it to exclusion list)
07:05:41.64 -01:30:01.5 -- not an asteroid (will add it to exclusion list)
07:01:59.75 -03:44:51.5 -- not an asteroid (will add it to exclusion list)
07:01:10.33 -01:01:15.8 -- not an asteroid (will add it to exclusion list)
06:54:15.84 -00:38:31.5 -- not an asteroid (will add it to exclusion list)
07:08:03.40 -03:34:26.0 -- not an asteroid (will add it to exclusion list)
07:07:00.65 -00:52:23.6 -- not an asteroid (will add it to exclusion list)
06:56:22.00 -00:53:11.7 -- not an asteroid (will add it to exclusion list)
07:01:00.38 -00:27:55.6 -- not an asteroid (will add it to exclusion list)
07:08:06.64 -05:59:32.1 -- not an asteroid (will add it to exclusion list)
06:59:02.37 -03:28:54.2 -- not an asteroid (will add it to exclusion list)
06:48:30.59 +00:57:43.9 -- not an asteroid (will add it to exclusion list)
07:04:33.71 -04:28:39.1 -- not an asteroid (will add it to exclusion list)
06:53:59.56 -01:59:29.4 -- not an asteroid (will add it to exclusion list)
06:57:09.52 -01:07:39.0 -- not an asteroid (will add it to exclusion list)
07:03:33.70 -02:51:42.1 -- not an asteroid (will add it to exclusion list)
06:59:44.18 -01:15:44.7 -- not an asteroid (will add it to exclusion list)
06:42:18.02 +00:54:40.1 -- not an asteroid (will add it to exclusion list)
06:55:24.16 -05:26:25.2 -- not an asteroid (will add it to exclusion list)
06:55:40.26 -02:20:14.6 -- not an asteroid (will add it to exclusion list)
06:34:41.23 -03:37:25.5 -- not an asteroid (will add it to exclusion list)
06:43:20.67 +02:08:46.3 -- not an asteroid (will add it to exclusion list)
07:08:56.42 -00:17:23.4 -- not an asteroid (will add it to exclusion list)
06:39:35.03 -04:06:33.0 -- not an asteroid (will add it to exclusion list)
07:09:11.07 -05:50:46.2 -- not an asteroid (will add it to exclusion list)
06:50:17.84 +02:13:22.6 -- not an asteroid (will add it to exclusion list)
06:52:06.23 -04:01:50.1 -- not an asteroid (will add it to exclusion list)
06:43:14.11 -00:36:30.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:34:41.23 -03:37:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:31.61 -01:23:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:35.03 -04:06:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:09.91 -03:38:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:18.02 +00:54:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:00.33 -00:24:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.11 -00:36:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:20.67 +02:08:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.51 +00:07:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:14.00 +00:50:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:30.59 +00:57:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:17.84 +02:13:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.23 -04:01:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:58.15 -04:52:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:59.56 -01:59:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.84 -00:38:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:24.16 -05:26:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:40.26 -02:20:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.00 -00:53:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.17 +00:46:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:48.11 -03:27:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:09.52 -01:07:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:49.24 -01:06:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:02.37 -03:28:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:44.18 -01:15:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:52.95 -04:47:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.84 -03:16:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.38 -00:27:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.30 +00:00:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.33 -01:01:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.09 -03:06:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.90 -06:08:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:27.45 -05:22:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:48.85 +01:06:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:59.75 -03:44:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.55 -03:05:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.53 -01:34:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:30.71 -03:26:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:50.48 -03:19:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.15 -02:49:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:33.70 -02:51:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:33.71 -04:28:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:39.00 -04:57:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:54.90 -01:47:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:55.92 +01:34:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:10.39 -00:29:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.74 +00:02:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:15.70 +00:02:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.16 -01:23:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.64 -01:30:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.76 -01:12:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:00.65 -00:52:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.54 -02:58:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:54.74 -02:07:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:03.40 -03:34:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:06.64 -05:59:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:21.63 -02:47:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.07 -01:45:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:56.42 -00:17:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:11.07 -05:50:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:34:41.23 -03:37:25.5 -- a known variable star
06:37:31.61 -01:23:43.5 -- a known variable star
06:39:35.03 -04:06:33.0 -- a known variable star
06:42:09.91 -03:38:13.0 -- not a known variable star
06:42:18.02 +00:54:40.1 -- a known variable star
06:43:00.33 -00:24:45.9 -- a known variable star
06:43:14.11 -00:36:30.4 -- a known variable star
06:43:20.67 +02:08:46.3 -- a known variable star
06:44:31.51 +00:07:32.9 -- not a known variable star
06:46:14.00 +00:50:46.5 -- not a known variable star
06:48:30.59 +00:57:43.9 -- not a known variable star
06:50:17.84 +02:13:22.6 -- a known variable star
06:52:06.23 -04:01:50.1 -- a known variable star
06:53:58.15 -04:52:50.3 -- not a known variable star
06:53:59.56 -01:59:29.4 -- not a known variable star
06:54:15.84 -00:38:31.5 -- not a known variable star
06:55:24.16 -05:26:25.2 -- a known variable star
06:55:40.26 -02:20:14.6 -- a known variable star
06:56:22.00 -00:53:11.7 -- a known variable star
06:56:45.17 +00:46:32.9 -- not a known variable star
06:56:48.11 -03:27:50.6 -- not a known variable star
06:57:09.52 -01:07:39.0 -- a known variable star
06:58:49.24 -01:06:26.0 -- a known variable star
06:59:02.37 -03:28:54.2 -- a known variable star
06:59:44.18 -01:15:44.7 -- not a known variable star
06:59:52.95 -04:47:25.5 -- not a known variable star
07:00:56.84 -03:16:18.6 -- not a known variable star
07:01:00.38 -00:27:55.6 -- a known variable star
07:01:10.30 +00:00:18.0 -- a known variable star
07:01:10.33 -01:01:15.8 -- not a known variable star
07:01:19.09 -03:06:46.3 -- not a known variable star
07:01:22.90 -06:08:19.4 -- not a known variable star
07:01:27.45 -05:22:48.4 -- not a known variable star
07:01:48.85 +01:06:04.8 -- not a known variable star
07:01:59.75 -03:44:51.5 -- not a known variable star
07:02:14.55 -03:05:58.7 -- not a known variable star
07:02:23.53 -01:34:45.2 -- not a known variable star
07:02:30.71 -03:26:38.2 -- not a known variable star
07:02:50.48 -03:19:42.3 -- a known variable star
07:03:24.15 -02:49:51.6 -- not a known variable star
07:03:33.70 -02:51:42.1 -- not a known variable star
07:04:33.71 -04:28:39.1 -- not a known variable star
07:04:39.00 -04:57:05.9 -- not a known variable star
07:04:54.90 -01:47:04.7 -- not a known variable star
07:04:55.92 +01:34:26.5 -- a known variable star
07:05:10.39 -00:29:31.3 -- a known variable star
07:05:14.74 +00:02:12.6 -- not a known variable star
07:05:15.70 +00:02:29.9 -- not a known variable star
07:05:18.16 -01:23:00.4 -- a known variable star
07:05:41.64 -01:30:01.5 -- not a known variable star
07:05:41.76 -01:12:42.3 -- not a known variable star
07:07:00.65 -00:52:23.6 -- not a known variable star
07:07:11.54 -02:58:22.4 -- not a known variable star
07:07:54.74 -02:07:28.1 -- not a known variable star
07:08:03.40 -03:34:26.0 -- a known variable star
07:08:06.64 -05:59:32.1 -- not a known variable star
07:08:21.63 -02:47:09.9 -- not a known variable star
07:08:44.07 -01:45:46.1 -- not a known variable star
07:08:56.42 -00:17:23.4 -- a known variable star
07:09:11.07 -05:50:46.2 -- a known variable star
Found 36 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
60 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 60 (excluding asteroids and hot pixels, 36 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)2461144.60745134 -observatory V36
23:57:26.85 -03:04:03.3 Mercury (0.1mag)
02:59:25.01 +17:08:08.1 Venus (-3.9mag)
00:12:27.76 +00:16:22.4 Mars (1.2mag)
07:11:47.38 +22:47:36.4 Jupiter (-2.1mag)
00:28:20.16 +00:43:42.4 Saturn (0.9mag)
03:47:18.09 +19:46:12.5 Uranus (5.8mag)
00:10:35.50 -00:16:56.3 Neptune (7.8mag)
20:33:40.11 -22:52:31.4 Pluto (14.5mag)
22:42:10.00 -08:19:52.9 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 13 21:43 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.60745134:
07:11:42.41 +22:47:48.4 Io (5.8mag)
07:11:47.49 +22:47:33.0 Europa (5.9mag)
07:11:54.87 +22:47:27.6 Ganymede (5.3mag)
07:12:13.14 +22:46:50.9 Callisto (6.6mag)
07:15:12.52 +22:36:07.3 Himalia (15.3mag)
07:11:45.07 +22:47:39.4 Thebe (16.2mag)
07:15:21.43 +23:06:09.6 Elara (17.3mag)
07:10:32.53 +23:28:36.1 Pasiphae (17.4mag)
07:20:09.58 +22:45:26.3 Carme (18.5mag)
00:28:28.35 +00:43:58.1 Titan (8.8mag)
00:28:22.66 +00:43:55.6 Rhea (10.1mag)
00:28:03.59 +00:44:09.9 Iapetus (11.5mag)
00:28:33.57 +00:43:50.9 Hyperion (14.8mag)
00:29:58.54 +00:52:42.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 21:43 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.60745134:
15:29:51.75 -14:52:20.9 JWST
16:53:52.16 +44:54:16.4 Chandra
07:50:05.89 -32:54:34.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 21:43 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.60745134 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:12.33 -28:40:07.4 13.9mag P/2010 H2 (Vales)
05:05:23.18 -69:45:07.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:02.60 +31:25:28.9 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.58 +10:19:23.0 17.6mag C/2021 G2 (ATLAS)
23:09:42.81 +29:09:16.2 17.1mag C/2022 E2 (ATLAS)
04:27:02.10 +25:59:13.1 16.0mag C/2022 N2 (PANSTARRS)
09:03:01.72 +32:00:18.9 16.2mag C/2022 QE78 (ATLAS)
08:30:47.59 -00:21:16.1 17.3mag C/2022 R6 (PANSTARRS)
18:54:10.13 +18:22:23.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:16.78 -11:32:57.2 17.5mag P/2023 B1 (PANSTARRS)
09:08:31.71 -12:11:15.0 17.6mag C/2023 F3 (ATLAS)
21:52:17.52 +62:47:47.0 17.5mag C/2023 H5 (Lemmon)
19:20:48.09 -03:42:08.5 14.2mag C/2023 R1 (PANSTARRS)
21:35:59.13 +85:39:00.3 17.8mag C/2023 X2 (Lemmon)
06:17:02.68 +63:31:19.9 17.1mag C/2024 A1 (ATLAS)
05:09:11.23 +17:39:59.1 10.9mag C/2024 E1 (Wierzchos)
16:20:28.94 +06:04:48.4 17.4mag C/2024 G6 (ATLAS)
20:20:16.12 +14:45:43.3 14.6mag C/2024 J3 (ATLAS)
03:24:40.38 -22:40:28.7 16.4mag C/2024 T5 (ATLAS)
05:15:06.78 +45:45:48.6 17.7mag C/2025 J1 (Borisov)
13:46:42.30 +44:12:32.3 15.1mag C/2025 L1 (ATLAS)
03:22:17.81 -25:55:05.1 17.8mag C/2025 Q3 (ATLAS)
23:28:18.51 +19:09:25.8 8.8mag C/2025 R3 (PANSTARRS)
12:54:56.40 +02:53:49.8 17.4mag C/2025 Y1 (ATLAS)
03:11:35.41 +02:50:35.0 12.7mag C/2026 A1 (MAPS)
23:54:11.28 +36:52:01.8 14.5mag C/2026 B2 (Sun-Gao)
18:39:14.97 -09:49:12.0 11.9mag 10P/Tempel
15:02:51.76 +03:24:12.3 13.8mag 24P/Schaumasse
11:03:19.01 -01:35:15.4 15.7mag 29P/Schwassmann-Wachmann
18:00:22.99 -09:40:48.8 17.9mag 40P/Vaisala
10:37:39.92 -04:15:03.2 16.9mag 43P/Wolf-Harrington
01:45:44.62 +17:09:53.1 17.2mag 47P/Ashbrook-Jackson
07:07:17.09 +37:25:08.3 17.0mag 63P/Wild
23:26:38.25 -11:40:43.3 15.7mag 65P/Gunn
03:58:12.23 +20:36:05.6 15.9mag 76P/West-Kohoutek-Ikemura
01:01:23.53 +07:51:23.3 14.3mag 78P/Gehrels
22:57:15.23 -09:57:02.7 14.6mag 88P/Howell
02:05:03.16 +20:08:10.4 15.1mag 93P/Lovas
04:51:14.83 +32:11:10.8 16.2mag 123P/West-Hartley
08:26:09.56 +39:14:05.1 16.2mag 124P/Mrkos
02:30:17.54 +14:09:30.9 16.4mag 128P/Shoemaker-Holt
02:43:49.47 +14:15:41.7 17.5mag 131P/Mueller
01:16:14.54 +12:34:43.0 10.7mag 141P/Machholz
01:25:25.82 +04:09:47.7 10.7mag 141P-A/Machholz
00:11:38.81 +00:08:38.1 13.0mag 141P-D/Machholz
01:55:35.62 +05:54:57.1 17.8mag 141P-I/Machholz
00:57:05.96 -02:28:38.8 15.1mag 162P/SidingSpring
10:29:06.68 +30:57:44.9 18.0mag 164P/Christensen
06:33:01.88 +24:18:06.1 18.0mag 198P/ODAS
14:54:48.04 -00:15:57.5 17.6mag 210P/Christensen
21:33:20.11 -11:54:18.2 17.6mag 218P/LINEAR
17:16:03.51 -14:09:35.9 16.1mag 235P/LINEAR
05:30:24.00 +34:33:13.1 16.7mag 240P/NEAT
07:37:34.44 -05:22:23.8 17.7mag 242P/Spahr
22:12:10.59 -21:28:49.2 17.9mag 260P/McNaught
15:43:22.34 +06:51:53.8 17.5mag 391P/Kowalski
07:33:28.75 +21:21:35.2 17.7mag 450P/LONEOS
05:33:06.95 +45:08:37.2 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 21:43 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 21:43 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 21:43 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 21:43 tns_transients_list.txt
