This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1111 Oph,2461136.8150,11.16,0.05,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
V1111 Oph 20260406.3150 11.16CV 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!
TCP 2026 04 06.3150* 18 45 09.83 +12 56 33.8 9.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184510+1256.6,2461136.8150,9.87,0.05,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
ASAS J184510+1256.6 20260406.3150 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190300+1610.4,2461136.8150,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190300+1610.4 20260406.3150 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.7842+15.9566,2461136.8150,13.80,0.05,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 J285.7842+15.9566 20260406.3150 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190458.04+181340.2,2461136.8150,13.38,0.05,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
ZTF J190458.04+181340.2 20260406.3150 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 57 32.55 +13 50 04.6 13.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.8150,13.14,0.05,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 20260406.3150 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.8150,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.3150 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4506111392966414336,2461136.8150,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4506111392966414336 20260406.3150 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 54 21.70 +14 50 21.6 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185422+1450.3,2461136.8150,11.36,0.05,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
ASAS J185422+1450.3 20260406.3150 11.36CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0675 Oph,2461136.8150,12.22,0.05,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
V0675 Oph 20260406.3150 12.22CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190038.46+155446.5,2461136.8150,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190038.46+155446.5 20260406.3150 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 46 37.77 +14 10 11.2 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11116145,2461136.8150,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11116145 20260406.3150 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183216+1102.9,2461136.8150,11.68,0.05,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
ASAS J183216+1102.9 20260406.3150 11.68CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0653 Oph,2461136.8150,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0653 Oph 20260406.3150 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 51 19.34 +13 52 17.5 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J185119.58+135223.0,2461136.8150,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J185119.58+135223.0 20260406.3150 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 50 18.90 +14 56 36.3 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11121745,2461136.8150,13.25,0.05,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
NSVS 11121745 20260406.3150 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184836.71+113738.8,2461136.8150,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184836.71+113738.8 20260406.3150 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J284.4661+09.9944,2461136.8150,12.86,0.05,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 J284.4661+09.9944 20260406.3150 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.1194+17.5080,2461136.8150,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.1194+17.5080 20260406.3150 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 55 45.88 +13 16 21.1 12.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185546.09+131620.7,2461136.8150,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185546.09+131620.7 20260406.3150 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.3150 2461136.8150 12.10 19:00:48.09 +13:59:18.2
46.45651 4.29831 galactic Aql Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4506513749839419648 | 19:00:48.31 +13:59:13.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 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 4506513749839419648,2461136.8150,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4506513749839419648 20260406.3150 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184824.71+105451.9,2461136.8150,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184824.71+105451.9 20260406.3150 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1900580+152243,2461136.8150,11.68,0.05,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
NSVS J1900580+152243 20260406.3150 11.68CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190119.67+140441.4,2461136.8150,12.80,0.05,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 J190119.67+140441.4 20260406.3150 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 53 26.88 +13 22 12.1 12.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11126155,2461136.8150,12.76,0.05,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
NSVS 11126155 20260406.3150 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190048.69+165302.7,2461136.8150,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190048.69+165302.7 20260406.3150 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J182844.93+105202.2,2461136.8150,12.61,0.05,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
ASASSN-V J182844.93+105202.2 20260406.3150 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 54 17.34 +13 54 53.6 13.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185417.58+135457.0,2461136.8150,13.37,0.05,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
ASASSN-V J185417.58+135457.0 20260406.3150 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190119.33+123435.4,2461136.8150,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190119.33+123435.4 20260406.3150 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1858107+161853,2461136.8150,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1858107+161853 20260406.3150 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IRAS 18587+1514,2461136.8150,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IRAS 18587+1514 20260406.3150 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185833+1614.4,2461136.8150,11.46,0.05,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
ASAS J185833+1614.4 20260406.3150 11.46CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0605 Oph,2461136.8150,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0605 Oph 20260406.3150 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0411 Oph,2461136.8150,12.43,0.05,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
V0411 Oph 20260406.3150 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.3150* 18 56 16.29 +12 58 40.5 10.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185616+1258.6,2461136.8150,10.86,0.05,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
ASAS J185616+1258.6 20260406.3150 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0677 Oph,2461136.8150,13.00,0.05,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
V0677 Oph 20260406.3150 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11106719,2461136.8150,12.93,0.05,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
NSVS 11106719 20260406.3150 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190213.04+174056.4,2461136.8150,13.17,0.05,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
ZTF J190213.04+174056.4 20260406.3150 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!
TCP 2026 04 06.3150* 18 49 10.56 +15 49 51.2 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184911+1549.9,2461136.8150,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184911+1549.9 20260406.3150 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190350.87+181218.3,2461136.8150,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190350.87+181218.3 20260406.3150 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4506918679331463296,2461136.8150,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4506918679331463296 20260406.3150 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.8014+13.8838,2461136.8150,13.19,0.05,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 J285.8014+13.8838 20260406.3150 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99633582 27.02.2026 11:54:33.415 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
First image: 2461098.99633582 27.02.2026 11:54:33.415 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Last image: 2461136.81524164 06.04.2026 07:33:46.878 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 4 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): 18710
Objects passed selection criteria: 18656
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: 15407.8
Average stars matched: 14981.5 (97.2335 %)
Memory usage VmPeak: 124532 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 02:36:02 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: 2461098.99633582 27.02.2026 11:54:33.415 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
First image: 2461098.99633582 27.02.2026 11:54:33.415 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Last image: 2461136.81524164 06.04.2026 07:33:46.878 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 262
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 59 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): 194732
Objects passed selection criteria: 194304
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 152414
Average stars matched: 146880 (96.3689 %)
Memory usage VmPeak: 2025492 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 02:41:38 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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: 2461136.81467531
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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits'
wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
Saving wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits to local_wcs_cache/
'wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits' -> 'local_wcs_cache/wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits'
wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits exists and is non-empty
Saving wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits to local_wcs_cache/
'wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits'
wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits exists and is non-empty
Saving wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits to local_wcs_cache/
'wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:00.619 +13:59:51.43
Second-epoch image center 18:39:59.053 +13:59:17.54
Angular distance between the image centers 0.0113 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 18:40:00.619 +13:59:51.43
Second-epoch image center 18:39:58.682 +13:58:49.33
Angular distance between the image centers 0.0189 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 18:39:59.053 +13:59:17.54
Second-epoch second image center 18:39:58.682 +13:58:49.33
Angular distance between the image centers 0.00798 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.tOLBA8Dyrh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.4GeTLTr4cD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits &> /tmp/tmp.UCLK18zV8y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits &> /tmp/tmp.CAjkNHsiS7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
Found non-empty wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
The reference image (wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits) and catalog (wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat) found
'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat' -> 'wcsmag.cat'
Read 23429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.6053 to 288.1585 deg, Dec +8.4734 to +19.3136 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 271.6053 to 288.1585 deg, Dec 8.4734 to 19.3136 deg
Loaded 15616 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): 9602 out of 10578 total matches.
Matched with Tycho-2 10578 out of 23429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.894388
a=0.000000 b=1.000000 c=22.894388
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
2.0 pix Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
2.8 pix fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
2.8 pix fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Limiting magnitude estimates:
15.0 mag. Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
15.0 mag. Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
14.1 mag. fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
14.1 mag. fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.tOLBA8Dyrh (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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2310, passed=23429
Got 23429 stars (including 21095 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 23429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 22687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 22687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 975 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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.4GeTLTr4cD (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/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits' -> 'wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2357, passed=23496
Got 23496 stars (including 21111 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 23496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 22626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 22626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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.UCLK18zV8y (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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=809, passed=11602
Got 11602 stars (including 10783 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 11602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 11500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 11498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 11498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits -region wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.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.CAjkNHsiS7 (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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=804, passed=11624
Got 11624 stars (including 10808 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 11624 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 11561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 11561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 957 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits -region wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits'
Saving fully-calibrated image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits'
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits'
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits'
Preparing the HTML report for the field Her-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out10127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31697.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 31693_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 31693_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:33.34 +13:26:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31694_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 31694_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:20:23.74 +12:39:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31695_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 31695_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:25:07.93 +12:43:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31696_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 31696_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:22:50.01 +10:42:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31697_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 31697_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 31698_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 31698_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:27:30.07 +15:41:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10127_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 10127_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 04465_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 04465_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:47:13.54 +10:33:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16528_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 16528_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 17789_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 17789_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:58:23.77 +16:46:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07604_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 07604_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:25:17.82 +11:37:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11114_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 11114_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:50:14.99 +13:25:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09119_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 09119_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:47:12.15 +12:27:23.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Her-10-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 ####
18:45:09.83 +12:56:33.8
19:02:59.59 +16:10:22.1
18:37:19.23 +10:25:48.6
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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:00.619 +13:59:51.43
Second-epoch image center 18:39:59.053 +13:59:17.54
Angular distance between the image centers 0.0113 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 18:40:00.619 +13:59:51.43
Second-epoch image center 18:39:58.682 +13:58:49.33
Angular distance between the image centers 0.0189 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 18:39:59.053 +13:59:17.54
Second-epoch second image center 18:39:58.682 +13:58:49.33
Angular distance between the image centers 0.00798 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.xopwafGHtw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.wy0kXLFj92
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits &> /tmp/tmp.rXPQSp3SKi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits &> /tmp/tmp.ya89KndzSn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
Found non-empty wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
The reference image (wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits) and catalog (wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat) found
'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat' -> 'wcsmag.cat'
Read 239572 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5882 to 288.1755 deg, Dec +8.4735 to +19.3174 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 271.5882 to 288.1755 deg, Dec 8.4735 to 19.3174 deg
Loaded 15640 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): 7671 out of 11356 total matches.
Matched with Tycho-2 11356 out of 239572 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.718977
a=0.000000 b=1.000000 c=22.718977
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 178 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
1.8 pix Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
2.5 pix fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
2.5 pix fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Limiting magnitude estimates:
15.2 mag. Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
15.2 mag. Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
14.2 mag. fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
14.2 mag. fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xopwafGHtw (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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=33427, passed=239534
Got 239534 stars (including 205755 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 239534 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 237477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 237478 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 237647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 968 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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.wy0kXLFj92 (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/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits' -> 'wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=33407, passed=239975
Got 239975 stars (including 206242 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 239975 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 237940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 237939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 237878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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.rXPQSp3SKi (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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=8400, passed=95665
Got 95665 stars (including 87172 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 95665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 94828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 94831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 94831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 953 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits -region wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.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.ya89KndzSn (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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=8628, passed=96989
Got 96989 stars (including 88263 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 96989 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 96055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 96057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 96057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits -region wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits
Saving fully-calibrated image wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-32-57_20.00sec_-4.90C_LIGHT_0266.fits
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.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_2026-04-06_CI_Her-10-Q2b1x1_023426_TTUQ2b1x1_11768_ybf01UJe/wcs_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267.fits
Preparing the HTML report for the field Her-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out146769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out163589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out252954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out271469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out43273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out104297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93338.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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: 20s
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Considering the candidate 271204_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 271204_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 271211_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271211_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:44:25.95 +12:56:23.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 271219_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271219_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:57:24.29 +16:17:28.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 271221_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271221_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:30.32 +15:56:35.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 271226_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271226_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:24:22.36 +12:59:39.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 271232_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271232_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:57:18.14 +13:07:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271236_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271236_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:53:02.56 +12:53:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.449 4506152766414626176 283.26092646138 +12.88817389978 12.9793 12.5324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271237_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 271237_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 271239_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 271239_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 271249_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271249_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:23:11.47 +13:09:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271254_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271254_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:53:11.34 +13:22:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271255_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271255_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:12.93 +12:04:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271257_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271257_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:21.10 +17:29:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271259_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271259_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:56:05.06 +11:26:36.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 271261_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271261_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:48:22.27 +11:48:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 271264_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271264_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:56:02.36 +13:05:54.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 271265_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 271265_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 271266_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271266_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:56:52.47 +12:39:45.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 271267_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271267_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:40:52.36 +10:37:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.249 4503953296488322944 280.21956864626 +10.61828181788 12.8267 11.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271272_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271272_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:20:18.21 +12:57:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.083 4485319426227075328 275.07609772355 +12.96680071298 13.2459 12.3021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271273_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271273_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:30:17.22 +10:57:26.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
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Considering the candidate 271277_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271277_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:40.44 +13:20:29.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
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Considering the candidate 271280_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 271280_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 271282_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271282_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:56:46.17 +10:14:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 271289_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271289_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:59:59.79 +12:35:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271290_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271290_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:29.18 +14:16:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.740 4506626548529371008 285.87264625197 +14.27388558792 11.9204 10.7338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271296_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271296_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:29.53 +14:41:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271297_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271297_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:45.71 +13:37:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271298_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271298_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:59:34.44 +12:19:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271302_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271302_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:01:57.72 +13:22:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271307_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271307_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:19.23 +17:01:18.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 271308_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271308_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:11:41.90 +15:40:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271309_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271309_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:01:11.50 +12:28:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271311_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271311_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:25.78 +16:27:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 5.400 4513796124584383872 285.85893034666 +16.45548856192 12.1669 11.2438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271314_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271314_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:14.27 +12:25:17.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)
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Considering the candidate 271316_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271316_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:20.01 +13:31:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.496 4314272211923113216 285.83349092981 +13.52537845467 12.3426 11.9308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271317_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271317_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:42.64 +12:50:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271318_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271318_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:49:59.27 +10:41:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271319_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271319_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:50:15.59 +10:27:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.792 4311618613677094528 282.56560365714 +10.46505710893 12.0517 11.2985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271320_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271320_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:05:11.23 +14:05:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.431 4506565117651565824 286.29784592127 +14.08516473445 11.7464 10.6455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271322_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271322_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:30.75 +12:09:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.543 4313667691023589120 285.12890270388 +12.15426402829 11.5714 10.4002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271324_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271324_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:49:11.72 +17:14:13.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)
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Considering the candidate 271326_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271326_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:00.63 +13:42:26.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.54, MAG_FAINT_SEARCH_LIMIT=10.52)
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Considering the candidate 271328_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271328_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:29:55.95 +09:50:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271334_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271334_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:57:22.33 +11:18:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271337_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271337_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:02:18.89 +15:06:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271341_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271341_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:54:34.15 +10:39:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271343_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271343_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:16.32 +11:26:49.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 271345_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271345_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:18:25.58 +13:00:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271347_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271347_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:51:31.77 +17:57:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271349_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271349_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:49.03 +17:53:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271350_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271350_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:18:04.02 +13:45:09.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 271354_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271354_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:29:45.22 +18:01:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271355_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271355_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:51:31.85 +10:17:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271358_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271358_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:59:18.90 +14:09:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271361_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271361_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:53:10.10 +09:49:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271362_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271362_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:57.99 +12:26:24.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 271365_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271365_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:20:45.62 +16:58:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.539 4522937292426872960 275.18997492999 +16.97260807123 13.1105 12.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271367_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271367_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:03.41 +13:28:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271368_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271368_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:01:54.42 +17:07:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.653 4514161540394629376 285.47721496625 +17.12522668635 12.2281 10.7656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271371_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271371_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:43:15.08 +09:59:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271374_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271374_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:54:48.61 +15:21:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271378_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271378_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:01:08.74 +15:41:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271383_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271383_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:24:22.20 +15:38:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271386_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271386_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:01.89 +13:59:18.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 271388_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271388_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:25:13.17 +11:00:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271391_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271391_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:54:41.10 +15:21:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.168 4507645628310786688 283.67191855979 +15.36723770897 13.4294 11.2853 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271393_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271393_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:14.46 +11:24:06.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 271396_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271396_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:17.55 +17:55:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.289 4524022063728243200 279.32333723925 +17.92609163311 13.5112 12.9777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271397_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271397_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:29.38 +17:51:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271400_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271400_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:51:08.16 +14:32:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271401_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271401_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:49:47.19 +15:55:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271404_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271404_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 271408_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271408_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:31:59.18 +15:32:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.643 4510113615292353792 277.99566849264 +15.53930270552 12.2633 10.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271409_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271409_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:46:27.13 +12:42:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271411_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271411_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:42:33.07 +17:42:31.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
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Considering the candidate 271412_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271412_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:32:45.96 +13:48:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271414_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271414_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:55:05.06 +16:43:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271418_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271418_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:22:17.84 +11:46:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271419_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271419_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:26:32.05 +14:55:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271422_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271422_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:27:52.92 +12:20:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271428_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271428_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 271429_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271429_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:11:58.82 +13:11:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.304 4497074682999309312 272.99504871991 +13.19747809553 13.7516 13.1765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271432_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271432_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:24:24.45 +09:59:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.570 4480368565885797248 276.10120536840 +09.99930996126 12.9730 10.8719 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271434_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271434_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:53:46.32 +17:15:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271435_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271435_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:34:57.29 +11:25:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271436_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271436_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:39:57.74 +14:08:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271438_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271438_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:36:42.25 +12:59:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271439_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271439_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:32:48.38 +17:17:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.919 4523888851023018112 278.20146828436 +17.29329723357 13.6255 13.0992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271441_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271441_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:50:20.84 +17:07:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.946 4511345519304438272 282.58727357977 +17.12775587269 13.7515 12.0680 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271442_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271442_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:58:07.66 +10:57:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.654 4311874245784931840 284.53306631795 +10.95396382703 12.5561 11.0404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271444_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271444_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:13:23.23 +13:25:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.217 4497108145079873664 273.34587303047 +13.41695466401 11.6871 10.1227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271447_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271447_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:43:20.36 +11:04:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.632 4503997895430248704 280.83450084262 +11.07681451533 12.8650 11.6071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271458_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271458_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:43:14.24 +12:38:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271464_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271464_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:31:02.83 +13:49:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 3.941 4508525065816858880 277.76291444212 +13.82159744185 14.1320 13.5139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271465_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271465_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:34:06.69 +17:17:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.661 4523880673405064704 278.52754339984 +17.28602546429 13.9165 13.3206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271469_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 271469_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:18:44.25 +13:53:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.753 4497457347406054528 274.68416933069 +13.88762289672 14.0272 13.2982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148424_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 148424_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 49854_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 49854_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:22:50.04 +10:42:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101935_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 101935_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:25:07.95 +12:43:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252298_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 252298_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:54:48.98 +10:04:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84286_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 84286_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:15:10.22 +11:56:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41710_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 41710_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 170570_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 170570_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 132949_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 132949_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 43273_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 43273_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:36:23.70 +10:34:21.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 56904_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 56904_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 72477_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 72477_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:57:38.73 +11:45:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73966_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 73966_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:25:17.83 +11:37:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126274_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 126274_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:49.29 +13:56:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109660_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 109660_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:59:18.44 +13:14:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115156_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 115156_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:59:47.28 +13:28:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196052_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 196052_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:21.94 +16:59:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55020_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 55020_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 124846_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 124846_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 169050_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 169050_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:27:30.11 +15:41:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150063_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 150063_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 69561_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 69561_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 174861_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 174861_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:02:05.25 +16:06:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.352 4513760115576891904 285.52300331850 +16.11399283373 12.4770 11.4828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96532_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 96532_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:00:55.26 +12:42:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26455_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 26455_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 200886_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 200886_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:58:23.76 +16:46:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163589_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 163589_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:49.35 +15:35:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.217 4512961938869951488 285.95712711090 +15.58560858433 12.1953 10.9521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92547_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 92547_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:47:12.15 +12:27:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89771_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 89771_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:42.14 +12:26:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181236_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 181236_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:31.59 +16:24:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99121_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 99121_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:44:27.96 +12:46:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113483_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 113483_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:19.70 +13:24:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235428_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 235428_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 23043_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 23043_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:41.44 +09:45:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110430_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 110430_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 127747_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 127747_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 224458_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 224458_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:05:00.74 +18:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229319_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 229319_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:27.55 +17:48:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50644_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 50644_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 258292_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 258292_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:42:24.62 +09:51:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146769_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 146769_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:30.21 +14:48:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.878 4506684204173860864 285.87725333842 +14.80485605187 12.2475 10.8944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42766_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 42766_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:47:13.54 +10:33:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159572_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 159572_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 230240_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 230240_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:32:58.47 +17:41:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129907_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 129907_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 100702_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 100702_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:20:23.73 +12:39:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105202_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 105202_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:45:09.83 +12:56:33.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 112813_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 112813_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 198620_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 198620_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 52372_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 52372_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 55929_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 55929_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:27:14.53 +11:00:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71103_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 71103_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:47:59.34 +11:41:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133891_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 133891_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:40:07.02 +14:11:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255477_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 255477_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:23:40.49 +11:04:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125738_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 125738_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 93338_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 93338_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 179589_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 179589_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 71661_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 71661_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:45:16.12 +11:42:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157520_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 157520_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 177960_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 177960_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 179639_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 179639_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:44:33.27 +16:19:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24291_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 24291_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 21948_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 21948_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 104297_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 104297_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 50199_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 50199_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 184328_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 184328_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:57:12.68 +16:34:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29730_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 29730_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 253312_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 253312_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 252954_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 252954_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:04:18.17 +14:15:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 33004_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 33004_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:28:59.56 +10:07:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117413_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 117413_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:50:14.98 +13:25:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169112_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 169112_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 252382_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 252382_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:02.05 +09:53:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252242_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 252242_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 252183_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 252183_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:38:21.82 +15:29:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252113_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 252113_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 153251_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 153251_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 252064_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 252064_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 131980_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 131980_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 19:03:28.58 +14:10:06.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251698_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 251698_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:52:27.77 +11:45:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41907_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 41907_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:37:19.29 +10:25:47.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251559_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267
The candidate 251559_fd_Her-10-Q2b1x1_2026-04-06_02-33-46_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 18:54:14.12 +17:58:26.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 59s
Prepared the HTML report for the field Her-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:45:09.83 +12:56:33.8
19:02:59.59 +16:10:22.1
18:37:19.23 +10:25:48.6
18:56:16.29 +12:58:40.5
18:55:45.88 +13:16:21.1
18:53:26.88 +13:22:12.1
18:51:19.34 +13:52:17.5
18:54:17.34 +13:54:53.6
19:00:48.09 +13:59:18.2
19:01:19.39 +14:04:39.0
18:46:37.77 +14:10:11.2
18:54:21.70 +14:50:21.6
18:50:18.90 +14:56:36.3
19:01:48.92 +15:05:37.4
19:00:59.37 +15:18:26.2
19:00:57.37 +15:22:43.8
18:49:10.56 +15:49:51.2
19:00:38.30 +15:54:46.2
18:58:32.55 +16:14:25.6
18:58:10.63 +16:18:49.6
19:00:48.71 +16:52:59.7
18:31:02.69 +09:40:15.1
19:04:30.24 +17:30:46.2
18:30:15.38 +09:46:12.6
19:03:12.36 +13:52:18.2
19:03:50.37 +18:12:14.6
19:02:12.60 +17:40:50.4
18:57:51.55 +09:59:43.2
19:03:10.43 +15:57:22.0
19:04:57.75 +18:13:35.9
18:57:32.55 +13:50:04.6
18:58:40.18 +17:19:05.7
18:59:21.04 +13:31:51.8
18:40:42.84 +10:03:41.6
18:44:20.56 +10:33:23.1
18:44:51.27 +10:53:21.5
18:48:24.62 +10:54:51.0
18:28:44.95 +10:52:02.2
18:38:43.59 +11:02:55.9
18:32:16.22 +11:02:55.2
18:48:36.57 +11:37:39.4
19:01:19.09 +12:34:35.4
########### Completed Her-10-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 ####
18:37:19.23 +10:25:48.6
18:45:09.83 +12:56:33.8
19:02:59.59 +16:10:22.1
19:03:10.43 +15:57:22.0
19:04:57.75 +18:13:35.9
18:57:32.55 +13:50:04.6
18:58:40.18 +17:19:05.7
18:59:21.04 +13:31:51.8
18:54:21.70 +14:50:21.6
18:44:20.56 +10:33:23.1
19:00:38.30 +15:54:46.2
18:46:37.77 +14:10:11.2
18:32:16.22 +11:02:55.2
18:38:43.59 +11:02:55.9
18:51:19.34 +13:52:17.5
18:50:18.90 +14:56:36.3
18:48:36.57 +11:37:39.4
18:57:51.55 +09:59:43.2
19:04:30.24 +17:30:46.2
18:55:45.88 +13:16:21.1
19:00:48.09 +13:59:18.2
18:48:24.62 +10:54:51.0
19:00:57.37 +15:22:43.8
19:01:19.39 +14:04:39.0
18:53:26.88 +13:22:12.1
19:00:48.71 +16:52:59.7
18:28:44.95 +10:52:02.2
18:54:17.34 +13:54:53.6
19:01:19.09 +12:34:35.4
18:58:10.63 +16:18:49.6
19:00:59.37 +15:18:26.2
18:58:32.55 +16:14:25.6
18:30:15.38 +09:46:12.6
18:31:02.69 +09:40:15.1
18:56:16.29 +12:58:40.5
18:44:51.27 +10:53:21.5
18:40:42.84 +10:03:41.6
19:02:12.60 +17:40:50.4
18:49:10.56 +15:49:51.2
19:03:50.37 +18:12:14.6
19:01:48.92 +15:05:37.4
19:03:12.36 +13:52:18.2
###################################################################################
18:37:19.23 +10:25:48.6 -- not an asteroid (will add it to exclusion list)
18:45:09.83 +12:56:33.8 -- not an asteroid (will add it to exclusion list)
19:02:59.59 +16:10:22.1 -- not an asteroid (will add it to exclusion list)
19:03:10.43 +15:57:22.0 -- not an asteroid (will add it to exclusion list)
19:04:57.75 +18:13:35.9 -- not an asteroid (will add it to exclusion list)
18:57:32.55 +13:50:04.6 -- not an asteroid (will add it to exclusion list)
18:58:40.18 +17:19:05.7 -- not an asteroid (will add it to exclusion list)
18:59:21.04 +13:31:51.8 -- not an asteroid (will add it to exclusion list)
18:54:21.70 +14:50:21.6 -- not an asteroid (will add it to exclusion list)
18:44:20.56 +10:33:23.1 -- not an asteroid (will add it to exclusion list)
19:00:38.30 +15:54:46.2 -- not an asteroid (will add it to exclusion list)
18:46:37.77 +14:10:11.2 -- not an asteroid (will add it to exclusion list)
18:32:16.22 +11:02:55.2 -- not an asteroid (will add it to exclusion list)
18:38:43.59 +11:02:55.9 -- not an asteroid (will add it to exclusion list)
18:51:19.34 +13:52:17.5 -- not an asteroid (will add it to exclusion list)
18:50:18.90 +14:56:36.3 -- not an asteroid (will add it to exclusion list)
18:48:36.57 +11:37:39.4 -- not an asteroid (will add it to exclusion list)
18:57:51.55 +09:59:43.2 -- not an asteroid (will add it to exclusion list)
19:04:30.24 +17:30:46.2 -- not an asteroid (will add it to exclusion list)
18:55:45.88 +13:16:21.1 -- not an asteroid (will add it to exclusion list)
19:00:48.09 +13:59:18.2 -- not an asteroid (will add it to exclusion list)
18:48:24.62 +10:54:51.0 -- not an asteroid (will add it to exclusion list)
19:00:57.37 +15:22:43.8 -- not an asteroid (will add it to exclusion list)
19:01:19.39 +14:04:39.0 -- not an asteroid (will add it to exclusion list)
18:53:26.88 +13:22:12.1 -- not an asteroid (will add it to exclusion list)
19:00:48.71 +16:52:59.7 -- not an asteroid (will add it to exclusion list)
18:28:44.95 +10:52:02.2 -- not an asteroid (will add it to exclusion list)
18:54:17.34 +13:54:53.6 -- not an asteroid (will add it to exclusion list)
19:01:19.09 +12:34:35.4 -- not an asteroid (will add it to exclusion list)
18:58:10.63 +16:18:49.6 -- not an asteroid (will add it to exclusion list)
19:00:59.37 +15:18:26.2 -- not an asteroid (will add it to exclusion list)
18:58:32.55 +16:14:25.6 -- not an asteroid (will add it to exclusion list)
18:30:15.38 +09:46:12.6 -- not an asteroid (will add it to exclusion list)
18:31:02.69 +09:40:15.1 -- not an asteroid (will add it to exclusion list)
18:56:16.29 +12:58:40.5 -- not an asteroid (will add it to exclusion list)
18:44:51.27 +10:53:21.5 -- not an asteroid (will add it to exclusion list)
18:40:42.84 +10:03:41.6 -- not an asteroid (will add it to exclusion list)
19:02:12.60 +17:40:50.4 -- not an asteroid (will add it to exclusion list)
18:49:10.56 +15:49:51.2 -- not an asteroid (will add it to exclusion list)
19:03:50.37 +18:12:14.6 -- not an asteroid (will add it to exclusion list)
19:01:48.92 +15:05:37.4 -- not an asteroid (will add it to exclusion list)
19:03:12.36 +13:52:18.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:28:44.95 +10:52:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:30:15.38 +09:46:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:31:02.69 +09:40:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:32:16.22 +11:02:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:19.23 +10:25:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:43.59 +11:02:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:40:42.84 +10:03:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:20.56 +10:33:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:51.27 +10:53:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:09.83 +12:56:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:37.77 +14:10:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:48:24.62 +10:54:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:48:36.57 +11:37:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:10.56 +15:49:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:18.90 +14:56:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:19.34 +13:52:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:26.88 +13:22:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:17.34 +13:54:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:21.70 +14:50:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:45.88 +13:16:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:16.29 +12:58:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:32.55 +13:50:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:51.55 +09:59:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:10.63 +16:18:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:32.55 +16:14:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:40.18 +17:19:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:21.04 +13:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:38.30 +15:54:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:48.09 +13:59:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:48.71 +16:52:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:57.37 +15:22:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:59.37 +15:18:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:19.09 +12:34:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:19.39 +14:04:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:48.92 +15:05:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:12.60 +17:40:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:59.59 +16:10:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:10.43 +15:57:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:12.36 +13:52:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:50.37 +18:12:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:30.24 +17:30:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:57.75 +18:13:35.9 -- 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)
18:28:44.95 +10:52:02.2 -- a known variable star
18:30:15.38 +09:46:12.6 -- a known variable star
18:31:02.69 +09:40:15.1 -- a known variable star
18:32:16.22 +11:02:55.2 -- a known variable star
18:37:19.23 +10:25:48.6 -- a known variable star
18:38:43.59 +11:02:55.9 -- a known variable star
18:40:42.84 +10:03:41.6 -- a known variable star
18:44:20.56 +10:33:23.1 -- a known variable star
18:44:51.27 +10:53:21.5 -- a known variable star
18:45:09.83 +12:56:33.8 -- a known variable star
18:46:37.77 +14:10:11.2 -- a known variable star
18:48:24.62 +10:54:51.0 -- a known variable star
18:48:36.57 +11:37:39.4 -- a known variable star
18:49:10.56 +15:49:51.2 -- a known variable star
18:50:18.90 +14:56:36.3 -- a known variable star
18:51:19.34 +13:52:17.5 -- a known variable star
18:53:26.88 +13:22:12.1 -- a known variable star
18:54:17.34 +13:54:53.6 -- a known variable star
18:54:21.70 +14:50:21.6 -- a known variable star
18:55:45.88 +13:16:21.1 -- a known variable star
18:56:16.29 +12:58:40.5 -- a known variable star
18:57:32.55 +13:50:04.6 -- not a known variable star
18:57:51.55 +09:59:43.2 -- not a known variable star
18:58:10.63 +16:18:49.6 -- a known variable star
18:58:32.55 +16:14:25.6 -- a known variable star
18:58:40.18 +17:19:05.7 -- not a known variable star
18:59:21.04 +13:31:51.8 -- not a known variable star
19:00:38.30 +15:54:46.2 -- a known variable star
19:00:48.09 +13:59:18.2 -- not a known variable star
19:00:48.71 +16:52:59.7 -- a known variable star
19:00:57.37 +15:22:43.8 -- a known variable star
19:00:59.37 +15:18:26.2 -- a known variable star
19:01:19.09 +12:34:35.4 -- a known variable star
19:01:19.39 +14:04:39.0 -- a known variable star
19:01:48.92 +15:05:37.4 -- not a known variable star
19:02:12.60 +17:40:50.4 -- a known variable star
19:02:59.59 +16:10:22.1 -- a known variable star
19:03:10.43 +15:57:22.0 -- not a known variable star
19:03:12.36 +13:52:18.2 -- not a known variable star
19:03:50.37 +18:12:14.6 -- a known variable star
19:04:30.24 +17:30:46.2 -- not a known variable star
19:04:57.75 +18:13:35.9 -- a known variable star
Found 9 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
42 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
18:28:44.95 +10:52:02.2
18:30:15.38 +09:46:12.6
18:31:02.69 +09:40:15.1
18:32:16.22 +11:02:55.2
18:37:19.23 +10:25:48.6
18:38:43.59 +11:02:55.9
18:40:42.84 +10:03:41.6
18:44:20.56 +10:33:23.1
18:44:51.27 +10:53:21.5
18:45:09.83 +12:56:33.8
18:46:37.77 +14:10:11.2
18:48:24.62 +10:54:51.0
18:48:36.57 +11:37:39.4
18:49:10.56 +15:49:51.2
18:50:18.90 +14:56:36.3
18:51:19.34 +13:52:17.5
18:53:26.88 +13:22:12.1
18:54:17.34 +13:54:53.6
18:54:21.70 +14:50:21.6
18:55:45.88 +13:16:21.1
18:56:16.29 +12:58:40.5
18:57:32.55 +13:50:04.6
18:57:51.55 +09:59:43.2
18:58:10.63 +16:18:49.6
18:58:32.55 +16:14:25.6
18:58:40.18 +17:19:05.7
18:59:21.04 +13:31:51.8
19:00:38.30 +15:54:46.2
19:00:48.09 +13:59:18.2
19:00:48.71 +16:52:59.7
19:00:57.37 +15:22:43.8
19:00:59.37 +15:18:26.2
19:01:19.09 +12:34:35.4
19:01:19.39 +14:04:39.0
19:01:48.92 +15:05:37.4
19:02:12.60 +17:40:50.4
19:02:59.59 +16:10:22.1
19:03:10.43 +15:57:22.0
19:03:12.36 +13:52:18.2
19:03:50.37 +18:12:14.6
19:04:30.24 +17:30:46.2
19:04:57.75 +18:13:35.9
19:03:30.21 +14:48:16.6
19:03:49.35 +15:35:07.9
19:02:05.25 +16:06:52.3
19:04:18.17 +14:15:19.3
18:44:25.95 +12:56:23.5
18:57:24.29 +16:17:28.7
19:00:30.32 +15:56:35.0
18:24:22.36 +12:59:39.8
18:53:02.56 +12:53:16.3
18:56:05.06 +11:26:36.9
18:48:22.27 +11:48:54.9
18:56:02.36 +13:05:54.5
18:56:52.47 +12:39:45.6
18:40:52.36 +10:37:04.1
18:20:18.21 +12:57:57.5
18:30:17.22 +10:57:26.2
18:52:40.44 +13:20:29.0
18:56:46.17 +10:14:15.1
19:03:29.18 +14:16:25.5
19:04:19.23 +17:01:18.9
19:03:25.78 +16:27:18.4
19:00:14.27 +12:25:17.7
19:03:20.01 +13:31:28.9
18:50:15.59 +10:27:52.6
19:05:11.23 +14:05:02.6
19:00:30.75 +12:09:13.1
18:49:11.72 +17:14:13.8
19:00:00.63 +13:42:26.7
19:04:57.99 +12:26:24.7
18:20:45.62 +16:58:21.0
19:01:54.42 +17:07:28.7
18:54:41.10 +15:21:59.9
18:37:17.55 +17:55:36.1
18:31:59.18 +15:32:18.1
18:42:33.07 +17:42:31.2
18:11:58.82 +13:11:51.2
18:24:24.45 +09:59:58.5
18:32:48.38 +17:17:36.7
18:50:20.84 +17:07:38.7
18:58:07.66 +10:57:12.0
18:13:23.23 +13:25:01.0
18:43:20.36 +11:04:35.4
18:31:02.83 +13:49:17.4
18:34:06.69 +17:17:10.9
18:18:44.25 +13:53:18.1
18:36:23.70 +10:34:21.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.81467531 -observatory V36
23:20:55.91 -06:23:07.0 Mercury (0.3mag)
02:22:04.54 +13:54:13.1 Venus (-3.9mag)
23:50:15.36 -02:10:19.1 Mars (1.2mag)
07:08:44.70 +22:52:22.6 Jupiter (-2.2mag)
00:24:49.00 +00:21:34.3 Saturn (0.9mag)
03:45:44.74 +19:41:10.0 Uranus (5.8mag)
00:09:32.77 -00:23:34.0 Neptune (7.8mag)
20:33:14.63 -22:52:29.2 Pluto (14.5mag)
16:04:12.45 -26:37:54.0 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 02:36 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461136.81467531:
07:08:45.34 +22:52:18.4 Io (5.7mag)
07:08:56.76 +22:51:56.7 Europa (5.8mag)
07:08:41.22 +22:52:36.8 Ganymede (5.3mag)
07:08:14.17 +22:53:16.0 Callisto (6.5mag)
07:12:27.43 +22:44:48.9 Himalia (15.3mag)
07:08:46.31 +22:52:21.5 Thebe (16.2mag)
07:12:25.29 +23:13:36.5 Elara (17.2mag)
07:06:58.04 +23:37:27.1 Pasiphae (17.3mag)
07:17:16.39 +22:49:19.6 Carme (18.4mag)
00:24:44.08 +00:21:34.7 Titan (8.8mag)
00:24:45.68 +00:21:47.6 Rhea (10.1mag)
00:24:49.30 +00:23:07.0 Iapetus (11.5mag)
00:24:51.21 +00:21:22.3 Hyperion (14.8mag)
00:26:33.15 +00:31:22.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 02:36 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.81467531:
14:47:32.78 -08:26:47.6 JWST
17:12:11.46 +44:03:52.6 Chandra
08:21:30.67 -44:55:15.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 02:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.81467531 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:11.87 -28:14:31.4 13.9mag P/2010 H2 (Vales)
05:00:09.84 -70:08:29.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:35.38 +31:22:35.8 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.70 +09:23:06.2 17.6mag C/2021 G2 (ATLAS)
23:07:23.52 +28:52:20.0 17.0mag C/2022 E2 (ATLAS)
04:18:07.88 +25:46:03.9 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.63 +31:54:30.9 16.1mag C/2022 QE78 (ATLAS)
08:29:59.64 -01:13:07.0 17.3mag C/2022 R6 (PANSTARRS)
18:55:34.33 +17:42:20.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:28.78 -11:39:32.0 17.6mag P/2023 B1 (PANSTARRS)
09:12:45.72 -13:28:56.1 17.5mag C/2023 F3 (ATLAS)
21:43:37.42 +62:22:39.2 17.5mag C/2023 H5 (Lemmon)
19:26:20.23 -03:36:34.9 14.3mag C/2023 R1 (PANSTARRS)
21:42:37.34 +84:37:35.1 17.8mag C/2023 X2 (Lemmon)
06:14:33.28 +63:34:56.2 17.0mag C/2024 A1 (ATLAS)
04:51:21.73 +14:36:34.7 10.4mag C/2024 E1 (Wierzchos)
16:25:02.16 +04:47:52.9 17.4mag C/2024 G6 (ATLAS)
20:17:35.82 +12:42:54.5 14.7mag C/2024 J3 (ATLAS)
03:17:52.32 -23:54:10.8 16.4mag C/2024 T5 (ATLAS)
05:08:48.04 +47:48:03.9 17.7mag C/2025 J1 (Borisov)
14:18:36.63 +37:30:56.5 14.8mag C/2025 L1 (ATLAS)
03:10:32.93 -24:45:58.9 17.8mag C/2025 Q3 (ATLAS)
22:53:54.10 +19:50:14.8 10.1mag C/2025 R3 (PANSTARRS)
12:58:20.24 +02:24:00.9 17.5mag C/2025 Y1 (ATLAS)
01:33:17.75 +04:39:36.5 7.3mag C/2026 A1 (MAPS)
23:31:11.01 +35:16:16.0 14.3mag C/2026 B2 (Sun-Gao)
18:24:01.92 -10:12:45.8 12.4mag 10P/Tempel
15:12:45.19 +04:06:08.4 13.1mag 24P/Schaumasse
11:05:43.71 -01:51:33.5 15.7mag 29P/Schwassmann-Wachmann
17:56:49.95 -09:59:17.2 17.7mag 40P/Vaisala
10:38:51.20 -04:56:11.9 16.7mag 43P/Wolf-Harrington
01:33:44.56 +15:49:03.2 17.1mag 47P/Ashbrook-Jackson
06:53:32.40 +39:03:17.9 17.0mag 63P/Wild
23:16:28.39 -12:38:22.5 15.7mag 65P/Gunn
03:37:59.47 +17:47:01.7 15.8mag 76P/West-Kohoutek-Ikemura
00:44:20.91 +06:18:35.0 14.4mag 78P/Gehrels
22:32:56.59 -12:14:08.9 14.5mag 88P/Howell
01:43:30.48 +17:58:55.9 15.1mag 93P/Lovas
04:37:08.56 +31:44:08.1 16.3mag 123P/West-Hartley
08:18:02.64 +42:50:00.6 16.2mag 124P/Mrkos
02:18:24.28 +13:16:16.2 16.4mag 128P/Shoemaker-Holt
02:28:38.31 +13:16:11.3 17.5mag 131P/Mueller
00:36:29.89 +09:39:29.3 11.2mag 141P/Machholz
00:46:27.82 +01:14:44.1 11.3mag 141P-A/Machholz
23:36:57.62 -02:23:03.8 14.0mag 141P-D/Machholz
01:15:36.29 +02:54:44.3 17.9mag 141P-I/Machholz
00:35:28.82 -06:21:25.5 15.2mag 162P/SidingSpring
10:30:56.05 +31:29:56.5 17.8mag 164P/Christensen
06:18:39.28 +24:31:12.1 17.8mag 198P/ODAS
15:08:29.22 -01:10:48.5 17.4mag 210P/Christensen
21:09:18.88 -13:47:30.7 17.4mag 218P/LINEAR
17:12:40.33 -15:03:34.6 16.2mag 235P/LINEAR
05:13:54.98 +33:52:03.7 16.6mag 240P/NEAT
07:34:14.82 -06:16:19.7 17.6mag 242P/Spahr
15:45:54.23 +06:19:05.5 17.5mag 391P/Kowalski
07:30:57.12 +21:18:45.3 17.6mag 450P/LONEOS
05:22:05.23 +45:36:13.5 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 02:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
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
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
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
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
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
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
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
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
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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 6 02:36 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:19:10.599 -33:29:33.62 AT 2026huk 2026-03-29.24 19.7
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
-rw-r--r-- 1 apache apache 30K Apr 6 02:36 tns_transients_list.txt
