This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.77,0.05,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 20260409.1145 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.79,0.05,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
target 20260409.1145 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0641451-005653,2461139.6145,13.76,0.05,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_J0641451-005653 20260409.1145 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J063959.17+005452.7,2461139.6145,13.71,0.05,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 J063959.17+005452.7 20260409.1145 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.70,0.05,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
target 20260409.1145 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119529893500368768,2461139.6145,13.71,0.05,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 3119529893500368768 20260409.1145 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.52,0.05,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
target 20260409.1145 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7805-02.2146,2461139.6145,13.61,0.05,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
ATO J099.7805-02.2146 20260409.1145 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.0643-00.0070,2461139.6145,13.52,0.05,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
ATO J101.0643-00.0070 20260409.1145 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.24,0.05,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
target 20260409.1145 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.6375-01.8671,2461139.6145,13.26,0.05,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 J101.6375-01.8671 20260409.1145 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107406673992729472,2461139.6145,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107406673992729472 20260409.1145 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119418288770129920,2461139.6145,13.13,0.05,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 3119418288770129920 20260409.1145 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,12.98,0.05,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 20260409.1145 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.7343+00.7248,2461139.6145,13.13,0.05,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 J100.7343+00.7248 20260409.1145 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.27,0.05,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
target 20260409.1145 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102673845,2461139.6145,12.97,0.05,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
CoRoT 102673845 20260409.1145 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.7700+01.0434,2461139.6145,12.81,0.05,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 J100.7700+01.0434 20260409.1145 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126679364782002048,2461139.6145,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126679364782002048 20260409.1145 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461139.6145,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260409.1145 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107032775621691520,2461139.6145,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107032775621691520 20260409.1145 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
CoRoT 102714427,2461139.6145,11.62,0.05,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
CoRoT 102714427 20260409.1145 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3071-00.0429,2461139.6145,10.54,0.05,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 J101.3071-00.0429 20260409.1145 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,12.29,0.05,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 20260409.1145 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 3126640293460604160,2461139.6145,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126640293460604160 20260409.1145 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103981287255761536,2461139.6145,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103981287255761536 20260409.1145 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.2775-01.0440,2461139.6145,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.2775-01.0440 20260409.1145 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461139.6145,12.46,0.05,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 J100.9580+01.5948 20260409.1145 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.3363-00.8503,2461139.6145,12.69,0.05,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 J100.3363-00.8503 20260409.1145 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6619-02.2718,2461139.6145,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6619-02.2718 20260409.1145 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,2461139.6145,12.64,0.05,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
target 20260409.1145 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5628-02.3059,2461139.6145,12.71,0.05,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 J101.5628-02.3059 20260409.1145 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.5106-00.8990,2461139.6145,12.65,0.05,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 J100.5106-00.8990 20260409.1145 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105621277567743360,2461139.6145,12.76,0.05,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 3105621277567743360 20260409.1145 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119467977252662016,2461139.6145,12.81,0.05,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 3119467977252662016 20260409.1145 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.9796-02.5682,2461139.6145,12.92,0.05,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 J098.9796-02.5682 20260409.1145 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
ATO J098.9690+00.8358,2461139.6145,12.94,0.05,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
ATO J098.9690+00.8358 20260409.1145 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
target,2461139.6145,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107281540128223104,2461139.6145,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107281540128223104 20260409.1145 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6933-02.7384,2461139.6145,12.92,0.05,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 J100.6933-02.7384 20260409.1145 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 3125637852391270784,2461139.6145,13.01,0.05,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 3125637852391270784 20260409.1145 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461139.6145,13.09,0.05,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
CoRoT 102785122 20260409.1145 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 J099.6630+01.9547,2461139.6145,13.19,0.05,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 J099.6630+01.9547 20260409.1145 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106831938650976384,2461139.6145,13.16,0.05,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 3106831938650976384 20260409.1145 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.1126-01.8057,2461139.6145,13.04,0.05,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 J100.1126-01.8057 20260409.1145 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.14,0.05,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 20260409.1145 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.19,0.05,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 20260409.1145 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.18,0.05,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 20260409.1145 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.22,0.05,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 20260409.1145 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1145 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125607134785759744,2461139.6145,13.20,0.05,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 3125607134785759744 20260409.1145 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.20,0.05,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 20260409.1145 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461139.6145,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9913-01.3476 20260409.1145 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104844811903742208,2461139.6145,13.16,0.05,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 3104844811903742208 20260409.1145 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.2592-02.8330,2461139.6145,13.29,0.05,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 J101.2592-02.8330 20260409.1145 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 09.1145 2461139.6145 13.51 06:38:53.85 -00:49:19.5
212.23376 -3.16498 galactic Mon Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3119330469578499072 | 06:38:54.14 -00:50:00.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1949AnHar.112....1C HD 291993
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3119330469578499072,2461139.6145,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3119330469578499072 20260409.1145 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106199856901798528,2461139.6145,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106199856901798528 20260409.1145 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3519-02.0494,2461139.6145,13.45,0.05,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 J101.3519-02.0494 20260409.1145 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.1014+01.3198,2461139.6145,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.1014+01.3198 20260409.1145 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12510161,2461139.6145,13.65,0.05,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 12510161 20260409.1145 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.3198+01.3769,2461139.6145,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.3198+01.3769 20260409.1145 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119728149190587520,2461139.6145,13.69,0.05,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 3119728149190587520 20260409.1145 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3519-02.0494,2461139.6145,13.70,0.05,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 J101.3519-02.0494 20260409.1145 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.91,0.05,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 20260409.1145 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4586-01.0450,2461139.6145,13.84,0.05,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 J100.4586-01.0450 20260409.1145 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6145,13.82,0.05,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 20260409.1145 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461139.61485521 09.04.2026 02:45:13.490 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
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: 7 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): 31452
Objects passed selection criteria: 31336
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 25148.8
Average stars matched: 22756.2 (90.4866 %)
Memory usage VmPeak: 131608 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:21:23 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: 2461139.61485521 09.04.2026 02:45:13.490 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 603
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: 203 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): 232316
Objects passed selection criteria: 231512
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 189458
Average stars matched: 171476 (90.509 %)
Memory usage VmPeak: 2217708 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:26:06 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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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: 2461139.61408554
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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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 06:51:23.409 -01:59:27.89
Angular distance between the image centers 0.0830 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 06:51:26.988 -02:00:05.57
Angular distance between the image centers 0.0671 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 06:51:23.409 -01:59:27.89
Second-epoch second image center 06:51:26.988 -02:00:05.57
Angular distance between the image centers 0.01821 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.yoQDvveBET
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.440n5fDCol
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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits &> /tmp/tmp.whVuHfWgzK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits &> /tmp/tmp.uO83Tpj2B8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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 19 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
2.5 pix fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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.yoQDvveBET (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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.440n5fDCol (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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.whVuHfWgzK (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2877, passed=28950
Got 28950 stars (including 26043 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 28950 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.3'
Seting catalog search parameters based on the expected field of view 924.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012837 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010270 (37.0 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 413 to 469 (Dec -7.3 to 3.6)
Done reading UCAC5 zone files...
Matched 508 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 429 matched stars entering correct_measured_positions(), 354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.10"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 423 matched stars entering correct_measured_positions(), 9730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.48"
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 3.6)
Done reading UCAC5 zone files...
Matched 546 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 475 matched stars entering correct_measured_positions(), 9751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.42"
Accuracy estimation diagnostic: 473 matched stars entering correct_measured_positions(), 11358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.44"
Excluding outliers - 473 stars left (next iteration limit 465)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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.uO83Tpj2B8 (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2893, passed=28815
Got 28815 stars (including 25893 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 28815 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 919.6'
Seting catalog search parameters based on the expected field of view 919.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012772 (46.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010218 (36.8 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 3.4)
Done reading UCAC5 zone files...
Matched 713 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 674 matched stars entering correct_measured_positions(), 616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 672 matched stars entering correct_measured_positions(), 16866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.24"
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 3.4)
Done reading UCAC5 zone files...
Matched 749 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 707 matched stars entering correct_measured_positions(), 16892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.20"
Accuracy estimation diagnostic: 703 matched stars entering correct_measured_positions(), 17551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.92"
Excluding outliers - 703 stars left (next iteration limit 739)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out56275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57982.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
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Considering the candidate 51878_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 51878_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (286.5") between the two second-epoch detections
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Considering the candidate 51880_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 51880_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (104.8") between the two second-epoch detections
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Considering the candidate 51884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 51884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (197.7") between the two second-epoch detections
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Considering the candidate 53644_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 53644_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (219.4") between the two second-epoch detections
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Considering the candidate 54799_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 54799_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:42:37.38 -03:49:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56275_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 56275_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:44:58.73 +00:57:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.080 3125630563829023488 101.24400728112 +00.95149061823 11.6686 11.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57158_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57158_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (71.4") between the two second-epoch detections
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Considering the candidate 57403_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57403_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (241.8") between the two second-epoch detections
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Considering the candidate 57411_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57411_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (200.1") between the two second-epoch detections
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Considering the candidate 57651_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57651_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (180.8") between the two second-epoch detections
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Considering the candidate 57656_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57656_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:42:36.18 -02:12:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.233 3106608119313089792 100.65078624539 -02.20722417901 11.9774 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57709_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57709_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:35:54.88 -03:57:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.652 3104828151726773888 098.97820694563 -03.96542848955 11.9193 11.4261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57758_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57758_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (124.4") between the two second-epoch detections
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Considering the candidate 57875_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57875_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:42:24.55 -02:50:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.857 3106502085160522880 100.60219933230 -02.83725286252 11.9149 11.4986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:36:08.23 -03:23:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.048 3104921713294147712 099.03374623654 -03.39027966343 12.0405 11.6214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57997_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 57997_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (148.2") between the two second-epoch detections
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Considering the candidate 58057_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 58057_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (125.1") between the two second-epoch detections
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Considering the candidate 58236_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 58236_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
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Considering the candidate 58309_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 58309_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (208.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 ####
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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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 06:51:23.409 -01:59:27.89
Angular distance between the image centers 0.0830 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 06:51:26.988 -02:00:05.57
Angular distance between the image centers 0.0671 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 06:51:23.409 -01:59:27.89
Second-epoch second image center 06:51:26.988 -02:00:05.57
Angular distance between the image centers 0.01821 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.gIHVyoZeYe
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.jU7snsuds6
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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits &> /tmp/tmp.h20t7zeBBd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits &> /tmp/tmp.rxfkBHufbs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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 514 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
2.3 pix fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gIHVyoZeYe (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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.jU7snsuds6 (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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.h20t7zeBBd (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=66, blended=31267, passed=199485
Got 199485 stars (including 167994 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 199485 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 924.3'
Seting catalog search parameters based on the expected field of view 924.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012837 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010270 (37.0 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 413 to 469 (Dec -7.3 to 3.6)
Done reading UCAC5 zone files...
Matched 493 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 422 matched stars entering correct_measured_positions(), 333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 419 matched stars entering correct_measured_positions(), 58130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
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 3.6)
Done reading UCAC5 zone files...
Matched 526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 477 matched stars entering correct_measured_positions(), 58152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Accuracy estimation diagnostic: 477 matched stars entering correct_measured_positions(), 71492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.32"
Excluding outliers - 477 stars left (next iteration limit 460)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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.rxfkBHufbs (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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=70, blended=32221, passed=203166
Got 203166 stars (including 170719 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 203166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 919.6'
Seting catalog search parameters based on the expected field of view 919.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012772 (46.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010218 (36.8 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 3.4)
Done reading UCAC5 zone files...
Matched 704 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 666 matched stars entering correct_measured_positions(), 608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 663 matched stars entering correct_measured_positions(), 122866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 732 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 697 matched stars entering correct_measured_positions(), 122885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.37"
Accuracy estimation diagnostic: 697 matched stars entering correct_measured_positions(), 128916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.02"
Excluding outliers - 697 stars left (next iteration limit 729)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/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_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-44-06_20.00sec_-4.90C_LIGHT_0048.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.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_2026-04-09_CI_Mon-02-Q2b1x1_011330_TTUQ2b1x1_8149_ZfiqF9lm/wcs_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out314871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out283601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out287362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328675.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 113s
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: 42s
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Considering the candidate 283589_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283589_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (127.6") between the two second-epoch detections
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Considering the candidate 283592_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283592_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (388.4") between the two second-epoch detections
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Considering the candidate 283597_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283597_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (195.9") between the two second-epoch detections
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Considering the candidate 283598_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283598_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (115.0") between the two second-epoch detections
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Considering the candidate 283601_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283601_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283608_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283608_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (125.9") between the two second-epoch detections
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Considering the candidate 283611_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283611_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283619_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283619_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283623_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283623_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283626_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (195.3") between the two second-epoch detections
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Considering the candidate 283627_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283627_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283628_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283628_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (177.4") between the two second-epoch detections
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Considering the candidate 283630_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283630_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (143.6") between the two second-epoch detections
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Considering the candidate 283632_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283632_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (223.8") between the two second-epoch detections
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Considering the candidate 283639_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283639_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (210.2") between the two second-epoch detections
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Considering the candidate 283642_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283642_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (107.1") between the two second-epoch detections
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Considering the candidate 283646_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283646_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283648_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283648_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (152.8") between the two second-epoch detections
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Considering the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283649_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (103.9") between the two second-epoch detections
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Considering the candidate 283655_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283655_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283659_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283659_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (163.7") between the two second-epoch detections
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Considering the candidate 283661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (341.6") between the two second-epoch detections
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Considering the candidate 283664_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283664_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (110.2") between the two second-epoch detections
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Considering the candidate 283666_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283666_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (106.4") between the two second-epoch detections
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Considering the candidate 283669_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283669_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (105.3") between the two second-epoch detections
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Considering the candidate 283672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (185.2") between the two second-epoch detections
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Considering the candidate 283673_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283673_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (99.6") between the two second-epoch detections
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Considering the candidate 283674_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283674_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (66.0") between the two second-epoch detections
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Considering the candidate 283677_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283677_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (159.1") between the two second-epoch detections
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Considering the candidate 283680_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283680_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (286.3") between the two second-epoch detections
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Considering the candidate 283687_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283687_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (142.7") between the two second-epoch detections
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Considering the candidate 283694_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283694_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (100.2") between the two second-epoch detections
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Considering the candidate 283696_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283696_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (294.1") between the two second-epoch detections
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Considering the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283700_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (145.7") between the two second-epoch detections
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Considering the candidate 283706_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283706_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (460.3") between the two second-epoch detections
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Considering the candidate 283710_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283710_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (204.2") between the two second-epoch detections
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Considering the candidate 283711_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283711_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (171.0") between the two second-epoch detections
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Considering the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283712_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (129.3") between the two second-epoch detections
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Considering the candidate 283721_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283721_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (156.8") between the two second-epoch detections
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Considering the candidate 283724_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283724_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (82.5") between the two second-epoch detections
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Considering the candidate 283729_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283729_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (132.5") between the two second-epoch detections
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Considering the candidate 283731_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283731_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (200.7") between the two second-epoch detections
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Considering the candidate 283732_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283732_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (161.0") between the two second-epoch detections
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Considering the candidate 283733_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283733_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (204.4") between the two second-epoch detections
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Considering the candidate 283735_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283735_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (472.8") between the two second-epoch detections
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Considering the candidate 283738_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283738_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (451.0") between the two second-epoch detections
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Considering the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283741_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (104.7") between the two second-epoch detections
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Considering the candidate 283742_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283742_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (226.3") between the two second-epoch detections
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Considering the candidate 283748_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283748_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283752_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (163.2") between the two second-epoch detections
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Considering the candidate 283753_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283753_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (169.2") between the two second-epoch detections
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Considering the candidate 283754_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283754_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283761_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283761_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (121.5") between the two second-epoch detections
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Considering the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283762_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (178.4") between the two second-epoch detections
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Considering the candidate 283764_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283764_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (210.8") between the two second-epoch detections
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Considering the candidate 283766_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283766_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (131.0") between the two second-epoch detections
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Considering the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283769_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (105.9") between the two second-epoch detections
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Considering the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283783_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283783_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (109.9") between the two second-epoch detections
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Considering the candidate 283786_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283786_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (323.9") between the two second-epoch detections
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Considering the candidate 283788_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283788_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283790_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283790_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (270.8") between the two second-epoch detections
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Considering the candidate 283792_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283792_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (120.1") between the two second-epoch detections
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Considering the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283794_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (196.5") between the two second-epoch detections
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Considering the candidate 283796_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283796_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (260.9") between the two second-epoch detections
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Considering the candidate 283798_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283798_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (134.4") between the two second-epoch detections
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Considering the candidate 283801_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283801_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (456.3") between the two second-epoch detections
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Considering the candidate 283802_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283802_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283803_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (135.6") between the two second-epoch detections
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Considering the candidate 283805_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283805_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (111.0") between the two second-epoch detections
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Considering the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283806_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (327.9") between the two second-epoch detections
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Considering the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (93.9") between the two second-epoch detections
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Considering the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283816_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (219.0") between the two second-epoch detections
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Considering the candidate 283822_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283822_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (47.7") between the two second-epoch detections
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Considering the candidate 283826_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283826_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.5") between the two second-epoch detections
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Considering the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283828_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (179.1") between the two second-epoch detections
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Considering the candidate 283829_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283829_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (289.5") between the two second-epoch detections
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Considering the candidate 283834_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283834_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (74.2") between the two second-epoch detections
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Considering the candidate 283845_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283845_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 283847_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283847_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (34.2") between the two second-epoch detections
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Considering the candidate 283848_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283848_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (244.8") between the two second-epoch detections
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Considering the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283849_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (303.1") between the two second-epoch detections
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Considering the candidate 283850_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283850_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (173.8") between the two second-epoch detections
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Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283852_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 283862_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283862_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (162.3") between the two second-epoch detections
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Considering the candidate 283863_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283863_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (270.5") between the two second-epoch detections
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Considering the candidate 283879_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283879_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (176.2") between the two second-epoch detections
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Considering the candidate 283882_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283882_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (110.0") between the two second-epoch detections
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Considering the candidate 283884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (146.2") between the two second-epoch detections
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Considering the candidate 283885_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283885_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (164.8") between the two second-epoch detections
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Considering the candidate 283889_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283889_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (375.6") between the two second-epoch detections
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Considering the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283895_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (65.3") between the two second-epoch detections
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Considering the candidate 283896_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283896_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (246.6") between the two second-epoch detections
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Considering the candidate 283898_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283898_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (275.3") between the two second-epoch detections
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Considering the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283902_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283902_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283903_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (97.3") between the two second-epoch detections
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Considering the candidate 283904_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283904_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (184.8") between the two second-epoch detections
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Considering the candidate 283909_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283909_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (164.6") between the two second-epoch detections
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Considering the candidate 283910_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283910_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 283912_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283912_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (277.9") between the two second-epoch detections
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Considering the candidate 283913_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283913_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (125.5") between the two second-epoch detections
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Considering the candidate 283915_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283915_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (150.1") between the two second-epoch detections
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Considering the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283918_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.0") between the two second-epoch detections
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Considering the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283922_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (209.0") between the two second-epoch detections
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Considering the candidate 283923_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283923_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283926_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283926_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (153.3") between the two second-epoch detections
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Considering the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283930_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283930_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (199.3") between the two second-epoch detections
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Considering the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283935_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283935_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (155.9") between the two second-epoch detections
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Considering the candidate 283936_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283936_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (355.0") between the two second-epoch detections
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Considering the candidate 283940_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283940_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (203.2") between the two second-epoch detections
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Considering the candidate 283941_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283941_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (66.1") between the two second-epoch detections
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Considering the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283945_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.7") between the two second-epoch detections
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Considering the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283946_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (184.6") between the two second-epoch detections
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Considering the candidate 283948_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283948_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (192.8") between the two second-epoch detections
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Considering the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283950_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (199.7") between the two second-epoch detections
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Considering the candidate 283952_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283952_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (148.7") between the two second-epoch detections
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Considering the candidate 283955_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283955_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (409.9") between the two second-epoch detections
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Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 283959_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283959_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (263.8") between the two second-epoch detections
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Considering the candidate 283960_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283960_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (106.5") between the two second-epoch detections
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Considering the candidate 283962_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283962_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (283.6") between the two second-epoch detections
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Considering the candidate 283964_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283964_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (230.5") between the two second-epoch detections
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Considering the candidate 283965_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283965_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (355.3") between the two second-epoch detections
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Considering the candidate 283967_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283967_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (291.9") between the two second-epoch detections
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Considering the candidate 283969_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283969_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (183.6") between the two second-epoch detections
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Considering the candidate 283972_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283972_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (284.5") between the two second-epoch detections
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Considering the candidate 283975_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283975_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (266.9") between the two second-epoch detections
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Considering the candidate 283978_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283978_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (391.3") between the two second-epoch detections
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Considering the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (195.5") between the two second-epoch detections
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Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283984_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (244.9") between the two second-epoch detections
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Considering the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283985_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (120.8") between the two second-epoch detections
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Considering the candidate 283990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (183.1") between the two second-epoch detections
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Considering the candidate 283992_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283992_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (271.7") between the two second-epoch detections
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Considering the candidate 283993_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283993_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (502.8") between the two second-epoch detections
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Considering the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283996_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (103.4") between the two second-epoch detections
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Considering the candidate 283997_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 283997_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (112.5") between the two second-epoch detections
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Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284000_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (237.1") between the two second-epoch detections
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Considering the candidate 284006_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284006_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (193.7") between the two second-epoch detections
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Considering the candidate 284007_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 284007_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 284008_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 284008_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 284011_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284011_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (101.1") between the two second-epoch detections
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Considering the candidate 284012_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284012_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (466.3") between the two second-epoch detections
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Considering the candidate 284013_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284013_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (366.8") between the two second-epoch detections
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Considering the candidate 284014_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284014_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (286.1") between the two second-epoch detections
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Considering the candidate 284018_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284018_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (296.5") between the two second-epoch detections
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Considering the candidate 284019_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284019_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (118.5") between the two second-epoch detections
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Considering the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284020_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (458.5") between the two second-epoch detections
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Considering the candidate 284022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (217.9") between the two second-epoch detections
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Considering the candidate 284024_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284024_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (145.7") between the two second-epoch detections
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Considering the candidate 284026_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284026_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (77.7") between the two second-epoch detections
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Considering the candidate 284028_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284028_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (295.2") between the two second-epoch detections
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Considering the candidate 284032_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284032_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (122.8") between the two second-epoch detections
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Considering the candidate 284035_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284035_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (369.5") between the two second-epoch detections
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Considering the candidate 284037_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284037_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (273.1") between the two second-epoch detections
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Considering the candidate 284040_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284040_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (108.6") between the two second-epoch detections
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Considering the candidate 284041_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284041_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (364.8") between the two second-epoch detections
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Considering the candidate 284045_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284045_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (151.1") between the two second-epoch detections
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Considering the candidate 284046_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284046_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (142.6") between the two second-epoch detections
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Considering the candidate 284048_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284048_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (207.5") between the two second-epoch detections
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Considering the candidate 284051_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284051_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (190.9") between the two second-epoch detections
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Considering the candidate 284052_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284052_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 284053_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284053_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (138.1") between the two second-epoch detections
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Considering the candidate 284055_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284055_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (267.4") between the two second-epoch detections
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Considering the candidate 284056_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284056_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (275.9") between the two second-epoch detections
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Considering the candidate 284059_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284059_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (381.3") between the two second-epoch detections
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Considering the candidate 284061_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284061_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (149.6") between the two second-epoch detections
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Considering the candidate 284062_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284062_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (127.9") between the two second-epoch detections
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Considering the candidate 284063_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284063_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (65.3") between the two second-epoch detections
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Considering the candidate 284066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (66.9") between the two second-epoch detections
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Considering the candidate 284067_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284067_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284069_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (94.3") between the two second-epoch detections
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Considering the candidate 284070_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284070_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (426.0") between the two second-epoch detections
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Considering the candidate 284077_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 284077_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 284078_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284078_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (230.8") between the two second-epoch detections
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Considering the candidate 284079_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284079_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.5") between the two second-epoch detections
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Considering the candidate 284080_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284080_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (131.0") between the two second-epoch detections
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Considering the candidate 284082_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284082_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (280.9") between the two second-epoch detections
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Considering the candidate 284083_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284083_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (467.4") between the two second-epoch detections
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Considering the candidate 284086_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 284086_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 284091_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284091_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (412.3") between the two second-epoch detections
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Considering the candidate 284096_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284096_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (101.8") between the two second-epoch detections
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Considering the candidate 284097_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284097_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (175.7") between the two second-epoch detections
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Considering the candidate 284098_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284098_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (180.0") between the two second-epoch detections
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Considering the candidate 284099_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284099_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (195.3") between the two second-epoch detections
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Considering the candidate 284101_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284101_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (310.3") between the two second-epoch detections
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Considering the candidate 284103_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284103_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (192.0") between the two second-epoch detections
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Considering the candidate 284104_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284104_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (256.0") between the two second-epoch detections
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Considering the candidate 284105_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284105_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (380.0") between the two second-epoch detections
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Considering the candidate 284106_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284106_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (103.5") between the two second-epoch detections
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Considering the candidate 284107_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284107_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (112.3") between the two second-epoch detections
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Considering the candidate 284110_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284110_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (140.5") between the two second-epoch detections
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Considering the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284112_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (216.2") between the two second-epoch detections
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Considering the candidate 284113_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284113_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (279.5") between the two second-epoch detections
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Considering the candidate 284115_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284115_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (262.6") between the two second-epoch detections
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Considering the candidate 284119_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 284119_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 284120_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284120_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (139.4") between the two second-epoch detections
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Considering the candidate 284121_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284121_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (259.1") between the two second-epoch detections
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Considering the candidate 284122_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284122_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (197.2") between the two second-epoch detections
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Considering the candidate 284124_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284124_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (93.9") between the two second-epoch detections
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Considering the candidate 284125_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284125_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (170.5") between the two second-epoch detections
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Considering the candidate 284126_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284126_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (173.3") between the two second-epoch detections
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Considering the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284127_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (411.4") between the two second-epoch detections
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Considering the candidate 284128_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284128_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (473.3") between the two second-epoch detections
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Considering the candidate 284129_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284129_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (254.9") between the two second-epoch detections
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Considering the candidate 284135_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284135_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (455.7") between the two second-epoch detections
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Considering the candidate 284137_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 284137_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (38.4") between the two second-epoch detections
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Considering the candidate 287143_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 287143_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (86.2") between the two second-epoch detections
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Considering the candidate 287362_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 287362_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 288136_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 288136_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (122.4") between the two second-epoch detections
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Considering the candidate 288782_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 288782_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (111.4") between the two second-epoch detections
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Considering the candidate 289134_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 289134_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (56.9") between the two second-epoch detections
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Considering the candidate 289463_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 289463_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (114.2") between the two second-epoch detections
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Considering the candidate 290126_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 290126_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (490.3") between the two second-epoch detections
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Considering the candidate 290479_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 290479_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:40:37.95 +00:43:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290914_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 290914_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:40:30.87 -01:04:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 292066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (458.5") between the two second-epoch detections
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Considering the candidate 292642_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 292642_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (86.4") between the two second-epoch detections
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Considering the candidate 292721_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 292721_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (287.7") between the two second-epoch detections
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Considering the candidate 294897_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 294897_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:43:32.96 -01:21:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 297813_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 297813_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (188.4") between the two second-epoch detections
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Considering the candidate 299448_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 299448_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 299741_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 299741_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:45:00.62 -00:03:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300400_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 300400_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 300461_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 300461_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 300587_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 300587_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (281.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301374_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 301374_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 302030_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302030_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.0") between the two second-epoch detections
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Considering the candidate 302131_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 302131_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302287_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302287_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (189.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302427_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 302427_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302530_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302530_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (481.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302862_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302862_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (464.1") between the two second-epoch detections
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Considering the candidate 302879_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302879_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (455.8") between the two second-epoch detections
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Considering the candidate 302903_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 302903_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (70.2") between the two second-epoch detections
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Considering the candidate 303192_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 303192_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (331.9") between the two second-epoch detections
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Considering the candidate 303559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 303559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (309.9") between the two second-epoch detections
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Considering the candidate 303767_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 303767_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 304640_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 304640_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (278.9") between the two second-epoch detections
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Considering the candidate 304702_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 304702_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (150.9") between the two second-epoch detections
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Considering the candidate 305204_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 305204_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (167.3") between the two second-epoch detections
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Considering the candidate 305386_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 305386_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (371.2") between the two second-epoch detections
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Considering the candidate 305791_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 305791_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (127.8") between the two second-epoch detections
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Considering the candidate 306021_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 306021_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (253.8") between the two second-epoch detections
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Considering the candidate 306342_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 306342_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 306844_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 306844_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 306990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 306990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 307137_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 307137_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 307559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 307559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (225.3") between the two second-epoch detections
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Considering the candidate 307618_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 307618_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (122.5") between the two second-epoch detections
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Considering the candidate 307939_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 307939_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (50.4") between the two second-epoch detections
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Considering the candidate 307982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 307982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (243.1") between the two second-epoch detections
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Considering the candidate 308141_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308141_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (126.5") between the two second-epoch detections
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Considering the candidate 308241_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308241_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (146.4") between the two second-epoch detections
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Considering the candidate 308266_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308266_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (99.0") between the two second-epoch detections
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Considering the candidate 308446_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308446_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (277.9") between the two second-epoch detections
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Considering the candidate 308500_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308500_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (152.1") between the two second-epoch detections
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Considering the candidate 308687_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 308687_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 308785_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308785_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (114.6") between the two second-epoch detections
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Considering the candidate 308822_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 308822_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (351.5") between the two second-epoch detections
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Considering the candidate 309062_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 309062_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (129.9") between the two second-epoch detections
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Considering the candidate 309203_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 309203_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 309406_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 309406_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (145.8") between the two second-epoch detections
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Considering the candidate 309853_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 309853_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (75.6") between the two second-epoch detections
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Considering the candidate 309949_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 309949_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (164.3") between the two second-epoch detections
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Considering the candidate 310049_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 310049_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (169.7") between the two second-epoch detections
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Considering the candidate 310175_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 310175_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 310608_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 310608_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (126.2") between the two second-epoch detections
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Considering the candidate 310615_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 310615_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (182.5") between the two second-epoch detections
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Considering the candidate 311003_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311003_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (90.9") between the two second-epoch detections
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Considering the candidate 311107_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311107_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (179.5") between the two second-epoch detections
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Considering the candidate 311183_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311183_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (162.2") between the two second-epoch detections
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Considering the candidate 311297_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 311297_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 311436_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311436_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (164.0") between the two second-epoch detections
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Considering the candidate 311503_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311503_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 311619_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311619_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (293.5") between the two second-epoch detections
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Considering the candidate 311675_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 311675_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 311684_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 311684_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 311760_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311760_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
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Considering the candidate 311774_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311774_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (148.6") between the two second-epoch detections
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Considering the candidate 311869_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311869_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (227.9") between the two second-epoch detections
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Considering the candidate 311905_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 311905_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 311928_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311928_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (102.9") between the two second-epoch detections
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Considering the candidate 311958_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311958_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (65.0") between the two second-epoch detections
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Considering the candidate 311990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311990_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (290.6") between the two second-epoch detections
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Considering the candidate 311999_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 311999_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.8") between the two second-epoch detections
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Considering the candidate 312179_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312179_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (118.5") between the two second-epoch detections
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Considering the candidate 312233_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312233_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (96.7") between the two second-epoch detections
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Considering the candidate 312248_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312248_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (110.8") between the two second-epoch detections
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Considering the candidate 312549_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312549_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (407.6") between the two second-epoch detections
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Considering the candidate 312616_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312616_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (136.3") between the two second-epoch detections
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Considering the candidate 312770_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 312770_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 312883_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 312883_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (38.5") between the two second-epoch detections
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Considering the candidate 313134_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313134_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (116.4") between the two second-epoch detections
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Considering the candidate 313138_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313138_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 313181_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313181_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (117.4") between the two second-epoch detections
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Considering the candidate 313626_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313626_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (89.2") between the two second-epoch detections
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Considering the candidate 313702_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313702_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (24.7") between the two second-epoch detections
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Considering the candidate 313809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 313818_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 313818_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 313840_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 313840_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 313847_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313847_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (131.3") between the two second-epoch detections
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Considering the candidate 313914_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313914_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (174.1") between the two second-epoch detections
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Considering the candidate 313964_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313964_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (287.1") between the two second-epoch detections
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Considering the candidate 313995_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 313995_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (75.6") between the two second-epoch detections
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Considering the candidate 314386_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314386_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (464.6") between the two second-epoch detections
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Considering the candidate 314583_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314583_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (363.4") between the two second-epoch detections
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Considering the candidate 314682_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314682_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (305.4") between the two second-epoch detections
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Considering the candidate 314823_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314823_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (114.3") between the two second-epoch detections
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Considering the candidate 314854_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314854_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (95.4") between the two second-epoch detections
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Considering the candidate 314871_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 314871_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:46:14.57 +00:45:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.194 3125565078465888768 101.55954576647 +00.75816110703 13.9059 12.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314966_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 314966_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 315167_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315167_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (153.7") between the two second-epoch detections
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Considering the candidate 315222_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 315222_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 315263_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315263_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (286.8") between the two second-epoch detections
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Considering the candidate 315662_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315662_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (150.4") between the two second-epoch detections
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Considering the candidate 315672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 315672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 315708_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315708_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (57.7") between the two second-epoch detections
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Considering the candidate 315825_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315825_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (99.6") between the two second-epoch detections
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Considering the candidate 315949_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 315949_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (78.8") between the two second-epoch detections
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Considering the candidate 316007_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 316007_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 316094_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316094_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (152.5") between the two second-epoch detections
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Considering the candidate 316333_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316333_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (359.5") between the two second-epoch detections
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Considering the candidate 316428_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316428_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (199.1") between the two second-epoch detections
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Considering the candidate 316569_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316569_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (212.9") between the two second-epoch detections
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Considering the candidate 316672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316672_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 316676_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316676_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (75.1") between the two second-epoch detections
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Considering the candidate 316772_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316772_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (192.5") between the two second-epoch detections
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Considering the candidate 316931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (70.6") between the two second-epoch detections
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Considering the candidate 316936_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 316936_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (118.8") between the two second-epoch detections
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Considering the candidate 317021_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317021_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (191.6") between the two second-epoch detections
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Considering the candidate 317034_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 317034_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 317133_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 317133_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317205_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317205_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (118.8") between the two second-epoch detections
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Considering the candidate 317235_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317235_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (272.6") between the two second-epoch detections
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Considering the candidate 317332_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317332_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (364.9") between the two second-epoch detections
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Considering the candidate 317347_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317347_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.2") between the two second-epoch detections
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Considering the candidate 317365_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 317365_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317497_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 317497_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317553_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 317553_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 318112_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318112_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (126.0") between the two second-epoch detections
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Considering the candidate 318144_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318144_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (168.8") between the two second-epoch detections
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Considering the candidate 318169_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 318169_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 318205_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318205_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (193.0") between the two second-epoch detections
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Considering the candidate 318221_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 318221_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 318259_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318259_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (108.6") between the two second-epoch detections
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Considering the candidate 318317_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318317_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 318449_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318449_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (241.8") between the two second-epoch detections
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Considering the candidate 318504_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318504_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (142.4") between the two second-epoch detections
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Considering the candidate 318551_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318551_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (108.5") between the two second-epoch detections
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Considering the candidate 318601_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318601_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (216.5") between the two second-epoch detections
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Considering the candidate 318869_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318869_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (137.1") between the two second-epoch detections
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Considering the candidate 318916_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318916_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (63.9") between the two second-epoch detections
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Considering the candidate 318970_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318970_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (139.9") between the two second-epoch detections
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Considering the candidate 318981_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 318981_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (304.0") between the two second-epoch detections
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Considering the candidate 319086_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 319086_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319133_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319133_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (261.2") between the two second-epoch detections
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Considering the candidate 319294_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319294_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (153.3") between the two second-epoch detections
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Considering the candidate 319313_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 319313_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 319391_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 319391_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 319473_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319473_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (159.4") between the two second-epoch detections
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Considering the candidate 319508_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319508_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (151.5") between the two second-epoch detections
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Considering the candidate 319693_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319693_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 319793_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319793_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (128.0") between the two second-epoch detections
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Considering the candidate 319807_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319807_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (153.6") between the two second-epoch detections
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Considering the candidate 319815_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 319815_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 319831_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 319831_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (165.8") between the two second-epoch detections
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Considering the candidate 320054_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320054_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (127.1") between the two second-epoch detections
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Considering the candidate 320222_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320222_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (65.1") between the two second-epoch detections
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Considering the candidate 320265_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320265_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (140.5") between the two second-epoch detections
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Considering the candidate 320267_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320267_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (179.4") between the two second-epoch detections
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Considering the candidate 320559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320559_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (90.6") between the two second-epoch detections
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Considering the candidate 320579_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320579_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (306.6") between the two second-epoch detections
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Considering the candidate 320878_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320878_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (272.4") between the two second-epoch detections
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Considering the candidate 320935_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320935_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (166.4") between the two second-epoch detections
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Considering the candidate 320939_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 320939_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (111.9") between the two second-epoch detections
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Considering the candidate 321096_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321096_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (121.0") between the two second-epoch detections
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Considering the candidate 321108_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321108_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
**** FOUND 06:38:52.78 +01:12:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.546 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321152_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321152_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (142.8") between the two second-epoch detections
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Considering the candidate 321361_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321361_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (137.9") between the two second-epoch detections
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Considering the candidate 321474_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321474_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (190.3") between the two second-epoch detections
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Considering the candidate 321524_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321524_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (80.8") between the two second-epoch detections
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Considering the candidate 321624_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321624_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (248.7") between the two second-epoch detections
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Considering the candidate 321646_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321646_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (329.2") between the two second-epoch detections
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Considering the candidate 321669_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321669_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (168.5") between the two second-epoch detections
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Considering the candidate 321791_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321791_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (92.6") between the two second-epoch detections
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Considering the candidate 321892_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 321892_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (115.6") between the two second-epoch detections
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Considering the candidate 322022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (47.0") between the two second-epoch detections
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Considering the candidate 322237_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322237_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (98.0") between the two second-epoch detections
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Considering the candidate 322262_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322262_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (37.1") between the two second-epoch detections
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Considering the candidate 322426_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 322426_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 322439_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322439_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (106.2") between the two second-epoch detections
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Considering the candidate 322561_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322561_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (241.8") between the two second-epoch detections
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Considering the candidate 322673_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322673_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (353.9") between the two second-epoch detections
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Considering the candidate 322764_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322764_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (97.6") between the two second-epoch detections
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Considering the candidate 322809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322809_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (146.7") between the two second-epoch detections
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Considering the candidate 322855_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 322855_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (154.9") between the two second-epoch detections
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Considering the candidate 323083_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323083_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (164.0") between the two second-epoch detections
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Considering the candidate 323233_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 323233_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 323246_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323246_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (298.7") between the two second-epoch detections
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Considering the candidate 323290_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323290_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (226.7") between the two second-epoch detections
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Considering the candidate 323308_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323308_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (108.1") between the two second-epoch detections
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Considering the candidate 323640_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323640_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (239.0") between the two second-epoch detections
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Considering the candidate 323641_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323641_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.1") between the two second-epoch detections
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Considering the candidate 323661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (141.1") between the two second-epoch detections
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Considering the candidate 323873_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323873_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (114.2") between the two second-epoch detections
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Considering the candidate 323884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 323884_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.2") between the two second-epoch detections
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Considering the candidate 324066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324066_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (63.3") between the two second-epoch detections
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Considering the candidate 324068_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324068_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (152.9") between the two second-epoch detections
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Considering the candidate 324139_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324139_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (162.6") between the two second-epoch detections
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Considering the candidate 324814_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 324814_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 324826_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324826_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (110.9") between the two second-epoch detections
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Considering the candidate 324829_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324829_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (220.6") between the two second-epoch detections
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Considering the candidate 324931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 324931_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (51.3") between the two second-epoch detections
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Considering the candidate 325047_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325047_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (119.6") between the two second-epoch detections
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Considering the candidate 325142_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325142_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (151.2") between the two second-epoch detections
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Considering the candidate 325247_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 325247_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 325306_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 325306_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 325335_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325335_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (226.6") between the two second-epoch detections
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Considering the candidate 325551_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325551_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.8") between the two second-epoch detections
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Considering the candidate 325627_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325627_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (153.1") between the two second-epoch detections
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Considering the candidate 325830_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 325830_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (350.1") between the two second-epoch detections
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Considering the candidate 325888_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 325888_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 325926_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 325926_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 326057_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326057_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 326176_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326176_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (177.4") between the two second-epoch detections
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Considering the candidate 326621_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326621_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (128.7") between the two second-epoch detections
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Considering the candidate 326636_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326636_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (213.6") between the two second-epoch detections
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Considering the candidate 326661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326661_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (95.0") between the two second-epoch detections
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Considering the candidate 326686_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326686_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (232.1") between the two second-epoch detections
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Considering the candidate 326724_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326724_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (127.1") between the two second-epoch detections
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Considering the candidate 326734_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 326734_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
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Considering the candidate 326746_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326746_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (38.4") between the two second-epoch detections
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Considering the candidate 326779_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326779_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 326816_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326816_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (486.7") between the two second-epoch detections
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Considering the candidate 326860_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326860_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (203.1") between the two second-epoch detections
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Considering the candidate 326861_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326861_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (221.8") between the two second-epoch detections
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Considering the candidate 326877_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326877_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (67.7") between the two second-epoch detections
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Considering the candidate 326889_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326889_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (149.4") between the two second-epoch detections
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Considering the candidate 326946_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326946_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (228.6") between the two second-epoch detections
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Considering the candidate 326982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 326982_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (138.4") between the two second-epoch detections
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Considering the candidate 327052_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327052_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (103.6") between the two second-epoch detections
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Considering the candidate 327147_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327147_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (113.2") between the two second-epoch detections
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Considering the candidate 327165_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327165_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (353.6") between the two second-epoch detections
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Considering the candidate 327219_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327219_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (117.5") between the two second-epoch detections
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Considering the candidate 327228_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327228_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (139.3") between the two second-epoch detections
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Considering the candidate 327287_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327287_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (190.5") between the two second-epoch detections
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Considering the candidate 327291_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327291_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (457.2") between the two second-epoch detections
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Considering the candidate 327349_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327349_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (250.4") between the two second-epoch detections
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Considering the candidate 327377_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327377_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (148.0") between the two second-epoch detections
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Considering the candidate 327423_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327423_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (367.0") between the two second-epoch detections
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Considering the candidate 327432_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327432_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (190.0") between the two second-epoch detections
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Considering the candidate 327460_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327460_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (379.4") between the two second-epoch detections
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Considering the candidate 327538_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327538_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (140.4") between the two second-epoch detections
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Considering the candidate 327583_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327583_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (128.7") between the two second-epoch detections
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Considering the candidate 327625_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327625_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (105.7") between the two second-epoch detections
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Considering the candidate 327719_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327719_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (90.6") between the two second-epoch detections
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Considering the candidate 327737_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327737_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (278.9") between the two second-epoch detections
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Considering the candidate 327789_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327789_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (165.2") between the two second-epoch detections
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Considering the candidate 327848_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327848_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (123.5") between the two second-epoch detections
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Considering the candidate 327852_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327852_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (183.8") between the two second-epoch detections
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Considering the candidate 327876_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327876_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (255.6") between the two second-epoch detections
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Considering the candidate 327895_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327895_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (216.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327930_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327930_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (110.5") between the two second-epoch detections
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Considering the candidate 327940_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327940_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (135.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327968_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327968_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (200.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327992_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 327992_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (138.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328005_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328005_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (101.0") between the two second-epoch detections
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Considering the candidate 328022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328022_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (276.2") between the two second-epoch detections
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Considering the candidate 328035_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328035_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (192.2") between the two second-epoch detections
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Considering the candidate 328081_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328081_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (105.3") between the two second-epoch detections
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Considering the candidate 328111_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328111_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (376.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328162_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328162_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (303.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328193_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328193_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (99.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328195_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328195_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (126.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328201_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328201_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (114.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328218_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328218_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (320.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328232_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328232_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (447.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328278_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328278_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 328293_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328293_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (333.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328309_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328309_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (58.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328347_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328347_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (181.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328371_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328371_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (145.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328374_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328374_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (135.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328411_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328411_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (377.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328446_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328446_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (30.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328450_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328450_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (97.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328461_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328461_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (160.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328477_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328477_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (147.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328484_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328484_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (191.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328494_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328494_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (461.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328547_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328547_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (209.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328578_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328578_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (290.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328590_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 328590_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328629_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 328629_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328649_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328649_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (323.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328675_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
Preparing report for the candidate 328675_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328679_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328679_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (116.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328728_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328728_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328770_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328770_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (117.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328783_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328783_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (188.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328849_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328849_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (202.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328886_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 328886_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (185.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329005_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 329005_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (156.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (201.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (189.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (57.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-08_21-45-13_20.00sec_-4.90C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (102.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 161s
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 ####
06:39:46.61 -02:14:04.0
06:42:51.67 -01:54:09.3
06:41:46.81 -00:57:12.8
06:41:20.96 +00:34:16.1
06:39:59.68 +00:54:50.6
06:42:17.47 +00:14:29.8
06:41:52.84 +00:02:59.9
06:42:01.52 +00:23:05.8
06:45:12.50 +00:14:12.3
06:39:07.86 -02:12:54.8
06:45:13.68 -00:39:29.8
06:44:12.88 -00:00:23.7
06:46:25.84 +00:47:28.6
06:46:33.15 -01:51:15.6
06:43:46.28 +00:35:14.4
06:46:26.15 -00:28:41.0
06:39:24.08 -00:23:31.0
06:38:38.02 -02:21:19.9
06:42:57.55 +00:43:54.2
06:38:54.91 +01:54:00.9
06:43:06.66 -00:47:40.3
06:43:05.11 +01:03:09.7
06:40:20.20 +01:45:33.2
06:35:07.87 -03:03:07.4
06:44:34.54 -01:35:32.6
06:43:57.87 +00:20:51.9
06:45:12.58 -00:01:54.1
06:38:54.68 +00:00:10.3
06:34:15.62 -05:19:06.6
06:40:14.10 +01:34:03.0
06:40:18.10 -04:25:59.9
06:45:05.28 -01:02:26.1
06:43:51.19 +01:35:48.2
06:41:18.96 -00:51:06.4
06:42:39.57 -02:16:11.5
06:45:06.57 -00:02:49.0
06:46:15.14 -02:18:27.8
06:41:58.50 -00:53:42.0
06:42:33.59 -03:28:08.6
06:41:47.49 -00:16:18.2
06:35:57.69 -02:34:27.7
06:35:50.84 +00:49:52.6
06:35:22.34 -05:17:41.2
06:42:42.72 -01:42:40.4
06:41:27.56 -01:19:07.0
06:42:46.93 -02:44:18.9
06:44:50.94 +01:05:42.8
06:45:34.20 -00:26:20.2
06:38:41.87 +01:56:34.2
06:41:21.51 -01:43:23.1
06:40:26.26 -01:49:10.5
06:35:10.89 -00:43:20.7
06:39:09.37 -03:48:13.9
06:40:17.66 -04:28:58.8
06:36:19.46 +00:01:22.8
06:35:12.05 -03:04:47.0
06:45:18.00 +00:43:35.8
06:44:20.36 +01:40:47.3
06:48:00.00 -01:20:59.3
06:36:32.90 -03:35:58.7
06:44:59.93 -02:49:34.9
06:38:53.85 -00:49:19.5
06:46:58.14 -02:12:27.2
06:45:25.11 -02:02:57.5
06:40:22.79 +01:18:18.6
06:37:19.72 +00:16:55.2
06:41:15.15 +01:21:50.9
06:39:28.88 +00:02:39.7
06:45:22.98 -02:01:53.7
06:43:24.24 -02:21:24.1
06:41:50.13 -01:02:44.1
06:44:44.44 +00:40:58.4
########### 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 ####
06:39:46.61 -02:14:04.0
06:42:51.67 -01:54:09.3
06:41:46.81 -00:57:12.8
06:41:20.96 +00:34:16.1
06:39:59.68 +00:54:50.6
06:42:17.47 +00:14:29.8
06:41:52.84 +00:02:59.9
06:42:01.52 +00:23:05.8
06:45:12.50 +00:14:12.3
06:39:07.86 -02:12:54.8
06:45:13.68 -00:39:29.8
06:44:12.88 -00:00:23.7
06:46:25.84 +00:47:28.6
06:46:33.15 -01:51:15.6
06:43:46.28 +00:35:14.4
06:46:26.15 -00:28:41.0
06:39:24.08 -00:23:31.0
06:38:38.02 -02:21:19.9
06:42:57.55 +00:43:54.2
06:38:54.91 +01:54:00.9
06:43:06.66 -00:47:40.3
06:43:05.11 +01:03:09.7
06:40:20.20 +01:45:33.2
06:35:07.87 -03:03:07.4
06:44:34.54 -01:35:32.6
06:43:57.87 +00:20:51.9
06:45:12.58 -00:01:54.1
06:38:54.68 +00:00:10.3
06:34:15.62 -05:19:06.6
06:40:14.10 +01:34:03.0
06:40:18.10 -04:25:59.9
06:45:05.28 -01:02:26.1
06:43:51.19 +01:35:48.2
06:41:18.96 -00:51:06.4
06:42:39.57 -02:16:11.5
06:45:06.57 -00:02:49.0
06:46:15.14 -02:18:27.8
06:41:58.50 -00:53:42.0
06:42:33.59 -03:28:08.6
06:41:47.49 -00:16:18.2
06:35:57.69 -02:34:27.7
06:35:50.84 +00:49:52.6
06:35:22.34 -05:17:41.2
06:42:42.72 -01:42:40.4
06:41:27.56 -01:19:07.0
06:42:46.93 -02:44:18.9
06:44:50.94 +01:05:42.8
06:45:34.20 -00:26:20.2
06:38:41.87 +01:56:34.2
06:41:21.51 -01:43:23.1
06:40:26.26 -01:49:10.5
06:35:10.89 -00:43:20.7
06:39:09.37 -03:48:13.9
06:40:17.66 -04:28:58.8
06:36:19.46 +00:01:22.8
06:35:12.05 -03:04:47.0
06:45:18.00 +00:43:35.8
06:44:20.36 +01:40:47.3
06:48:00.00 -01:20:59.3
06:36:32.90 -03:35:58.7
06:44:59.93 -02:49:34.9
06:38:53.85 -00:49:19.5
06:46:58.14 -02:12:27.2
06:45:25.11 -02:02:57.5
06:40:22.79 +01:18:18.6
06:37:19.72 +00:16:55.2
06:41:15.15 +01:21:50.9
06:39:28.88 +00:02:39.7
06:45:22.98 -02:01:53.7
06:43:24.24 -02:21:24.1
06:41:50.13 -01:02:44.1
06:44:44.44 +00:40:58.4
###################################################################################
06:39:46.61 -02:14:04.0 -- not an asteroid (will add it to exclusion list)
06:42:51.67 -01:54:09.3 -- not an asteroid (will add it to exclusion list)
06:41:46.81 -00:57:12.8 -- not an asteroid (will add it to exclusion list)
06:41:20.96 +00:34:16.1 -- not an asteroid (will add it to exclusion list)
06:39:59.68 +00:54:50.6 -- not an asteroid (will add it to exclusion list)
06:42:17.47 +00:14:29.8 -- not an asteroid (will add it to exclusion list)
06:41:52.84 +00:02:59.9 -- not an asteroid (will add it to exclusion list)
06:42:01.52 +00:23:05.8 -- not an asteroid (will add it to exclusion list)
06:45:12.50 +00:14:12.3 -- not an asteroid (will add it to exclusion list)
06:39:07.86 -02:12:54.8 -- not an asteroid (will add it to exclusion list)
06:45:13.68 -00:39:29.8 -- not an asteroid (will add it to exclusion list)
06:44:12.88 -00:00:23.7 -- not an asteroid (will add it to exclusion list)
06:46:25.84 +00:47:28.6 -- not an asteroid (will add it to exclusion list)
06:46:33.15 -01:51:15.6 -- not an asteroid (will add it to exclusion list)
06:43:46.28 +00:35:14.4 -- not an asteroid (will add it to exclusion list)
06:46:26.15 -00:28:41.0 -- not an asteroid (will add it to exclusion list)
06:39:24.08 -00:23:31.0 -- not an asteroid (will add it to exclusion list)
06:38:38.02 -02:21:19.9 -- not an asteroid (will add it to exclusion list)
06:42:57.55 +00:43:54.2 -- not an asteroid (will add it to exclusion list)
06:38:54.91 +01:54:00.9 -- not an asteroid (will add it to exclusion list)
06:43:06.66 -00:47:40.3 -- not an asteroid (will add it to exclusion list)
06:43:05.11 +01:03:09.7 -- not an asteroid (will add it to exclusion list)
06:40:20.20 +01:45:33.2 -- not an asteroid (will add it to exclusion list)
06:35:07.87 -03:03:07.4 -- not an asteroid (will add it to exclusion list)
06:44:34.54 -01:35:32.6 -- not an asteroid (will add it to exclusion list)
06:43:57.87 +00:20:51.9 -- not an asteroid (will add it to exclusion list)
06:45:12.58 -00:01:54.1 -- not an asteroid (will add it to exclusion list)
06:38:54.68 +00:00:10.3 -- not an asteroid (will add it to exclusion list)
06:34:15.62 -05:19:06.6 -- not an asteroid (will add it to exclusion list)
06:40:14.10 +01:34:03.0 -- not an asteroid (will add it to exclusion list)
06:40:18.10 -04:25:59.9 -- not an asteroid (will add it to exclusion list)
06:45:05.28 -01:02:26.1 -- not an asteroid (will add it to exclusion list)
06:43:51.19 +01:35:48.2 -- not an asteroid (will add it to exclusion list)
06:41:18.96 -00:51:06.4 -- not an asteroid (will add it to exclusion list)
06:42:39.57 -02:16:11.5 -- not an asteroid (will add it to exclusion list)
06:45:06.57 -00:02:49.0 -- not an asteroid (will add it to exclusion list)
06:46:15.14 -02:18:27.8 -- not an asteroid (will add it to exclusion list)
06:41:58.50 -00:53:42.0 -- not an asteroid (will add it to exclusion list)
06:42:33.59 -03:28:08.6 -- not an asteroid (will add it to exclusion list)
06:41:47.49 -00:16:18.2 -- not an asteroid (will add it to exclusion list)
06:35:57.69 -02:34:27.7 -- not an asteroid (will add it to exclusion list)
06:35:50.84 +00:49:52.6 -- not an asteroid (will add it to exclusion list)
06:35:22.34 -05:17:41.2 -- not an asteroid (will add it to exclusion list)
06:42:42.72 -01:42:40.4 -- not an asteroid (will add it to exclusion list)
06:41:27.56 -01:19:07.0 -- not an asteroid (will add it to exclusion list)
06:42:46.93 -02:44:18.9 -- not an asteroid (will add it to exclusion list)
06:44:50.94 +01:05:42.8 -- not an asteroid (will add it to exclusion list)
06:45:34.20 -00:26:20.2 -- not an asteroid (will add it to exclusion list)
06:38:41.87 +01:56:34.2 -- not an asteroid (will add it to exclusion list)
06:41:21.51 -01:43:23.1 -- not an asteroid (will add it to exclusion list)
06:40:26.26 -01:49:10.5 -- not an asteroid (will add it to exclusion list)
06:35:10.89 -00:43:20.7 -- not an asteroid (will add it to exclusion list)
06:39:09.37 -03:48:13.9 -- not an asteroid (will add it to exclusion list)
06:40:17.66 -04:28:58.8 -- not an asteroid (will add it to exclusion list)
06:36:19.46 +00:01:22.8 -- not an asteroid (will add it to exclusion list)
06:35:12.05 -03:04:47.0 -- not an asteroid (will add it to exclusion list)
06:45:18.00 +00:43:35.8 -- not an asteroid (will add it to exclusion list)
06:44:20.36 +01:40:47.3 -- not an asteroid (will add it to exclusion list)
06:48:00.00 -01:20:59.3 -- not an asteroid (will add it to exclusion list)
06:36:32.90 -03:35:58.7 -- not an asteroid (will add it to exclusion list)
06:44:59.93 -02:49:34.9 -- not an asteroid (will add it to exclusion list)
06:38:53.85 -00:49:19.5 -- not an asteroid (will add it to exclusion list)
06:46:58.14 -02:12:27.2 -- not an asteroid (will add it to exclusion list)
06:45:25.11 -02:02:57.5 -- not an asteroid (will add it to exclusion list)
06:40:22.79 +01:18:18.6 -- not an asteroid (will add it to exclusion list)
06:37:19.72 +00:16:55.2 -- not an asteroid (will add it to exclusion list)
06:41:15.15 +01:21:50.9 -- not an asteroid (will add it to exclusion list)
06:39:28.88 +00:02:39.7 -- not an asteroid (will add it to exclusion list)
06:45:22.98 -02:01:53.7 -- not an asteroid (will add it to exclusion list)
06:43:24.24 -02:21:24.1 -- not an asteroid (will add it to exclusion list)
06:41:50.13 -01:02:44.1 -- not an asteroid (will add it to exclusion list)
06:44:44.44 +00:40:58.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:34:15.62 -05:19:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:07.87 -03:03:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:10.89 -00:43:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:12.05 -03:04:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:22.34 -05:17:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:50.84 +00:49:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:57.69 -02:34:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:19.46 +00:01:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:32.90 -03:35:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:19.72 +00:16:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:38.02 -02:21:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:41.87 +01:56:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:53.85 -00:49:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:54.68 +00:00:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:54.91 +01:54:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:07.86 -02:12:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:09.37 -03:48:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:24.08 -00:23:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:28.88 +00:02:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:46.61 -02:14:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:59.68 +00:54:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:14.10 +01:34:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:17.66 -04:28:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:18.10 -04:25:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:20.20 +01:45:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:22.79 +01:18:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:26.26 -01:49:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:15.15 +01:21:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:18.96 -00:51:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:20.96 +00:34:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.51 -01:43:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.56 -01:19:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:46.81 -00:57:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:47.49 -00:16:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:50.13 -01:02:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:52.84 +00:02:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:58.50 -00:53:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:01.52 +00:23:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:17.47 +00:14:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.59 -03:28:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:39.57 -02:16:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.72 -01:42:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:46.93 -02:44:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:51.67 -01:54:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:57.55 +00:43:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:05.11 +01:03:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:06.66 -00:47:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:24.24 -02:21:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.28 +00:35:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:51.19 +01:35:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:57.87 +00:20:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:12.88 -00:00:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:20.36 +01:40:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.54 -01:35:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:44.44 +00:40:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.94 +01:05:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:59.93 -02:49:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:05.28 -01:02:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:06.57 -00:02:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.50 +00:14:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.58 -00:01:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:13.68 -00:39:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:18.00 +00:43:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:22.98 -02:01:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:25.11 -02:02:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:34.20 -00:26:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:15.14 -02:18:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.84 +00:47:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:26.15 -00:28:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:33.15 -01:51:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:58.14 -02:12:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:00.00 -01:20:59.3 -- 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)
06:34:15.62 -05:19:06.6 -- not a known variable star
06:35:07.87 -03:03:07.4 -- not a known variable star
06:35:10.89 -00:43:20.7 -- not a known variable star
06:35:12.05 -03:04:47.0 -- not a known variable star
06:35:22.34 -05:17:41.2 -- not a known variable star
06:35:50.84 +00:49:52.6 -- not a known variable star
06:35:57.69 -02:34:27.7 -- not a known variable star
06:36:19.46 +00:01:22.8 -- not a known variable star
06:36:32.90 -03:35:58.7 -- not a known variable star
06:37:19.72 +00:16:55.2 -- a known variable star
06:38:38.02 -02:21:19.9 -- not a known variable star
06:38:41.87 +01:56:34.2 -- not a known variable star
06:38:53.85 -00:49:19.5 -- not a known variable star
06:38:54.68 +00:00:10.3 -- not a known variable star
06:38:54.91 +01:54:00.9 -- not a known variable star
06:39:07.86 -02:12:54.8 -- not a known variable star
06:39:09.37 -03:48:13.9 -- not a known variable star
06:39:24.08 -00:23:31.0 -- not a known variable star
06:39:28.88 +00:02:39.7 -- a known variable star
06:39:46.61 -02:14:04.0 -- not a known variable star
06:39:59.68 +00:54:50.6 -- a known variable star
06:40:14.10 +01:34:03.0 -- not a known variable star
06:40:17.66 -04:28:58.8 -- not a known variable star
06:40:18.10 -04:25:59.9 -- a known variable star
06:40:20.20 +01:45:33.2 -- not a known variable star
06:40:22.79 +01:18:18.6 -- not a known variable star
06:40:26.26 -01:49:10.5 -- not a known variable star
06:41:15.15 +01:21:50.9 -- not a known variable star
06:41:18.96 -00:51:06.4 -- not a known variable star
06:41:20.96 +00:34:16.1 -- not a known variable star
06:41:21.51 -01:43:23.1 -- not a known variable star
06:41:27.56 -01:19:07.0 -- a known variable star
06:41:46.81 -00:57:12.8 -- not a known variable star
06:41:47.49 -00:16:18.2 -- not a known variable star
06:41:50.13 -01:02:44.1 -- not a known variable star
06:41:52.84 +00:02:59.9 -- a known variable star
06:41:58.50 -00:53:42.0 -- not a known variable star
06:42:01.52 +00:23:05.8 -- not a known variable star
06:42:17.47 +00:14:29.8 -- not a known variable star
06:42:33.59 -03:28:08.6 -- not a known variable star
06:42:39.57 -02:16:11.5 -- not a known variable star
06:42:42.72 -01:42:40.4 -- not a known variable star
06:42:46.93 -02:44:18.9 -- not a known variable star
06:42:51.67 -01:54:09.3 -- not a known variable star
06:42:57.55 +00:43:54.2 -- not a known variable star
06:43:05.11 +01:03:09.7 -- not a known variable star
06:43:06.66 -00:47:40.3 -- a known variable star
06:43:24.24 -02:21:24.1 -- not a known variable star
06:43:46.28 +00:35:14.4 -- not a known variable star
06:43:51.19 +01:35:48.2 -- not a known variable star
06:43:57.87 +00:20:51.9 -- a known variable star
06:44:12.88 -00:00:23.7 -- not a known variable star
06:44:20.36 +01:40:47.3 -- not a known variable star
06:44:34.54 -01:35:32.6 -- a known variable star
06:44:44.44 +00:40:58.4 -- not a known variable star
06:44:50.94 +01:05:42.8 -- not a known variable star
06:44:59.93 -02:49:34.9 -- not a known variable star
06:45:05.28 -01:02:26.1 -- not a known variable star
06:45:06.57 -00:02:49.0 -- not a known variable star
06:45:12.50 +00:14:12.3 -- not a known variable star
06:45:12.58 -00:01:54.1 -- not a known variable star
06:45:13.68 -00:39:29.8 -- not a known variable star
06:45:18.00 +00:43:35.8 -- not a known variable star
06:45:22.98 -02:01:53.7 -- not a known variable star
06:45:25.11 -02:02:57.5 -- not a known variable star
06:45:34.20 -00:26:20.2 -- a known variable star
06:46:15.14 -02:18:27.8 -- not a known variable star
06:46:25.84 +00:47:28.6 -- not a known variable star
06:46:26.15 -00:28:41.0 -- not a known variable star
06:46:33.15 -01:51:15.6 -- not a known variable star
06:46:58.14 -02:12:27.2 -- not a known variable star
06:48:00.00 -01:20:59.3 -- not a known variable star
Found 62 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
72 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 72 (excluding asteroids and hot pixels, 62 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)2461139.61408554 -observatory V36
23:33:14.99 -05:21:28.9 Mercury (0.2mag)
02:35:22.33 +15:06:33.0 Venus (-3.9mag)
23:58:14.72 -01:17:35.6 Mars (1.2mag)
07:09:45.60 +22:50:49.6 Jupiter (-2.1mag)
00:26:05.21 +00:29:35.5 Saturn (0.9mag)
03:46:17.44 +19:42:56.5 Uranus (5.8mag)
00:09:55.52 -00:21:09.4 Neptune (7.8mag)
20:33:24.54 -22:52:27.0 Pluto (14.5mag)
18:33:08.22 -27:54:08.2 Moon (-10.7mag)
-rw-r--r-- 1 apache apache 362 Apr 9 01:21 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461139.61408554:
07:09:48.90 +22:50:45.4 Io (5.7mag)
07:09:53.07 +22:50:36.6 Europa (5.9mag)
07:10:01.07 +22:50:13.5 Ganymede (5.3mag)
07:09:14.65 +22:51:54.8 Callisto (6.5mag)
07:13:22.51 +22:41:48.7 Himalia (15.3mag)
07:09:49.75 +22:50:41.5 Thebe (16.2mag)
07:13:24.46 +23:11:09.8 Elara (17.3mag)
07:08:10.34 +23:34:26.2 Pasiphae (17.4mag)
07:18:14.01 +22:48:06.9 Carme (18.5mag)
00:26:11.68 +00:29:24.7 Titan (8.8mag)
00:26:10.16 +00:29:43.7 Rhea (10.1mag)
00:25:59.11 +00:30:47.3 Iapetus (11.5mag)
00:26:16.44 +00:29:21.7 Hyperion (14.8mag)
00:27:47.35 +00:39:07.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 01:21 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.61408554:
15:04:17.43 -10:54:02.6 JWST
17:28:54.73 +39:43:41.0 Chandra
16:41:04.38 -53:31:47.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 01:21 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.61408554 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:46.01 -28:23:25.7 13.9mag P/2010 H2 (Vales)
05:01:58.58 -69:59:54.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:04.39 +31:23:35.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.70 +09:43:26.0 17.6mag C/2021 G2 (ATLAS)
23:08:15.84 +28:58:08.0 17.0mag C/2022 E2 (ATLAS)
04:21:17.92 +25:50:51.7 15.9mag C/2022 N2 (PANSTARRS)
09:02:12.35 +31:57:06.9 16.2mag C/2022 QE78 (ATLAS)
08:30:12.96 -00:54:07.3 17.3mag C/2022 R6 (PANSTARRS)
18:55:08.40 +17:56:49.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:44.73 -11:37:13.7 17.6mag P/2023 B1 (PANSTARRS)
09:11:08.30 -13:00:36.5 17.6mag C/2023 F3 (ATLAS)
21:46:52.31 +62:31:17.3 17.5mag C/2023 H5 (Lemmon)
19:24:32.12 -03:38:16.1 14.2mag C/2023 R1 (PANSTARRS)
21:41:20.02 +84:58:59.0 17.8mag C/2023 X2 (Lemmon)
06:15:15.36 +63:33:25.4 17.1mag C/2024 A1 (ATLAS)
04:57:57.91 +15:47:26.5 10.6mag C/2024 E1 (Wierzchos)
16:23:28.67 +05:15:31.0 17.4mag C/2024 G6 (ATLAS)
20:18:37.96 +13:26:19.5 14.7mag C/2024 J3 (ATLAS)
03:20:16.83 -23:27:18.1 16.4mag C/2024 T5 (ATLAS)
05:11:00.84 +47:03:06.2 17.7mag C/2025 J1 (Borisov)
14:07:21.02 +40:10:58.0 14.9mag C/2025 L1 (ATLAS)
03:14:40.50 -25:10:13.6 17.8mag C/2025 Q3 (ATLAS)
23:02:34.80 +19:46:30.6 9.6mag C/2025 R3 (PANSTARRS)
12:57:07.14 +02:34:55.3 17.5mag C/2025 Y1 (ATLAS)
02:16:29.88 +03:44:53.6 10.3mag C/2026 A1 (MAPS)
23:39:35.59 +35:52:20.9 14.4mag C/2026 B2 (Sun-Gao)
18:29:30.22 -10:04:35.8 12.2mag 10P/Tempel
15:09:21.26 +03:52:09.0 13.4mag 24P/Schaumasse
11:04:48.72 -01:45:31.6 15.7mag 29P/Schwassmann-Wachmann
17:58:19.13 -09:52:29.1 17.8mag 40P/Vaisala
10:38:17.17 -04:40:48.5 16.8mag 43P/Wolf-Harrington
01:38:02.48 +16:18:16.6 17.2mag 47P/Ashbrook-Jackson
06:58:21.90 +38:28:25.0 17.0mag 63P/Wild
23:20:09.59 -12:17:26.0 15.7mag 65P/Gunn
03:45:08.98 +18:49:06.5 15.9mag 76P/West-Kohoutek-Ikemura
00:50:26.28 +06:52:02.8 14.4mag 78P/Gehrels
22:41:47.52 -11:25:12.3 14.6mag 88P/Howell
01:51:09.62 +18:46:03.7 15.1mag 93P/Lovas
04:42:06.52 +31:54:10.9 16.3mag 123P/West-Hartley
08:20:46.30 +41:32:29.2 16.2mag 124P/Mrkos
02:22:38.80 +13:35:34.1 16.4mag 128P/Shoemaker-Holt
02:34:04.46 +13:37:57.8 17.5mag 131P/Mueller
00:50:33.24 +10:44:19.2 11.0mag 141P/Machholz
01:00:17.73 +02:17:16.3 11.0mag 141P-A/Machholz
23:49:10.69 -01:29:50.4 13.7mag 141P-D/Machholz
01:29:51.74 +03:59:45.2 17.9mag 141P-I/Machholz
00:43:13.69 -04:58:18.8 15.2mag 162P/SidingSpring
10:30:07.10 +31:19:26.1 17.9mag 164P/Christensen
06:23:47.30 +24:27:03.4 17.9mag 198P/ODAS
15:03:38.00 -00:50:08.4 17.4mag 210P/Christensen
21:18:11.04 -13:06:54.0 17.5mag 218P/LINEAR
17:14:07.36 -14:44:36.4 16.2mag 235P/LINEAR
05:19:46.52 +34:07:48.7 16.6mag 240P/NEAT
07:35:21.41 -05:56:25.4 17.7mag 242P/Spahr
15:45:04.94 +06:31:09.0 17.5mag 391P/Kowalski
07:31:46.88 +21:20:00.3 17.6mag 450P/LONEOS
05:25:59.30 +45:26:15.7 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 01:21 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 01:21 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:50:17.550 +33:04:52.33 AT 2026ifp 2026-03-27.86 19.99
16:52:21.140 +31:25:32.03 AT 2026ifo 2026-03-27.86 19.73
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
16:26:20.250 +28:06:35.30 AT 2026ifm 2026-03-27.85 20.13
17:01:36.800 +29:43:13.81 AT 2026ifl 2026-03-27.85 20.62
17:06:26.770 +28:47:25.16 AT 2026ifk 2026-03-27.85 21.39
16:47:18.680 +27:13:25.92 AT 2026ifj 2026-03-27.85 20.26
15:55:49.720 +37:36:32.33 AT 2026ifi 2026-03-24.80 21.32
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
16:30:53.670 +55:47:08.39 AT 2026ife 2026-03-30.85 20.99
16:07:35.060 +52:45:21.40 AT 2026ifd 2026-03-30.82 20.79
12:49:57.980 +19:52:49.93 AT 2026ifc 2026-03-20.70 19.71
15:58:08.890 +36:23:36.27 AT 2026ifb 2026-03-18.81 20.34
15:47:02.670 +48:09:28.72 AT 2026ifa 2026-03-30.81 20.31
15:30:58.600 +53:17:16.37 AT 2026iez 2026-03-23.80 21.21
10:25:53.600 +03:15:54.45 AT 2026iey 2026-03-24.63 22.18
19:10:17.892 -22:37:27.97 AT 2026iex 2026-03-30.80 18.87
12:44:39.935 -44:03:37.93 AT 2026iew 2026-03-31.50 19.02
-rw-r--r-- 1 apache apache 30K Apr 9 01:21 tns_transients_list.txt
