This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD
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
target,2461138.8374,12.95,0.05,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 20260408.3374 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
ATO J304.0534+31.1029,2461138.8374,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.0534+31.1029 20260408.3374 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1835433284465028224,2461138.8374,12.78,0.05,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
Gaia DR3 1835433284465028224 20260408.3374 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
ASASSN-V J200110.84+322116.4,2461138.8374,12.96,0.05,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 J200110.84+322116.4 20260408.3374 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194106.92+282140.4,2461138.8374,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194106.92+282140.4 20260408.3374 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.6914+28.0109,2461138.8374,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.6914+28.0109 20260408.3374 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2058263502094820480,2461138.8374,12.72,0.05,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
Gaia DR3 2058263502094820480 20260408.3374 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2025422193635409536,2461138.8374,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2025422193635409536 20260408.3374 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.5242+30.2188,2461138.8374,13.03,0.05,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 J293.5242+30.2188 20260408.3374 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2044734806109646464,2461138.8374,13.38,0.05,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
Gaia DR3 2044734806109646464 20260408.3374 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!
Don'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 1837324994211337344,2461138.8374,13.05,0.05,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
Gaia DR3 1837324994211337344 20260408.3374 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 J195637.90+265839.7,2461138.8374,13.17,0.05,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
ASASSN-V J195637.90+265839.7 20260408.3374 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195724.58+270317.5,2461138.8374,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195724.58+270317.5 20260408.3374 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IO Cyg,2461138.8374,12.83,0.05,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
IO Cyg 20260408.3374 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J200724.74+324515.6,2461138.8374,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200724.74+324515.6 20260408.3374 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201952.79+321923.8,2461138.8374,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201952.79+321923.8 20260408.3374 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1146 Cyg,2461138.8374,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1146 Cyg 20260408.3374 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.3530+33.4245,2461138.8374,12.88,0.05,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 J301.3530+33.4245 20260408.3374 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.8374,13.02,0.05,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 20260408.3374 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8363904,2461138.8374,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8363904 20260408.3374 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193822.53+293335.9,2461138.8374,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193822.53+293335.9 20260408.3374 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201333.28+325149.2,2461138.8374,13.03,0.05,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 J201333.28+325149.2 20260408.3374 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8374,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3374 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200910.22+293751.5,2461138.8374,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200910.22+293751.5 20260408.3374 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195214.26+302630.6,2461138.8374,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195214.26+302630.6 20260408.3374 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.9268+26.0131,2461138.8374,12.61,0.05,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
ATO J304.9268+26.0131 20260408.3374 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2004 Cyg,2461138.8374,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2004 Cyg 20260408.3374 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195045.00+290222.6,2461138.8374,13.08,0.05,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 J195045.00+290222.6 20260408.3374 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201923.27+285932.0,2461138.8374,12.14,0.05,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
ASASSN-V J201923.27+285932.0 20260408.3374 12.14CV 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
ASASSN-V J201712.80+275149.4,2461138.8374,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201712.80+275149.4 20260408.3374 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1837136084373516672,2461138.8374,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1837136084373516672 20260408.3374 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201947.30+264806.3,2461138.8374,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201947.30+264806.3 20260408.3374 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200206.74+280940.3,2461138.8374,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200206.74+280940.3 20260408.3374 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8451676,2461138.8374,12.95,0.05,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
NSVS 8451676 20260408.3374 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
ZTF J200720.94+284343.5,2461138.8374,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200720.94+284343.5 20260408.3374 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201411.42+272458.9,2461138.8374,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201411.42+272458.9 20260408.3374 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194502.04+291505.7,2461138.8374,12.80,0.05,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
ASASSN-V J194502.04+291505.7 20260408.3374 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!
Don'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
HAT 199-05667,2461138.8374,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05667 20260408.3374 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2920 Cyg,2461138.8374,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2920 Cyg 20260408.3374 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 1861556065829617920,2461138.8374,12.61,0.05,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
Gaia DR3 1861556065829617920 20260408.3374 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201946.97+334022.4,2461138.8374,12.93,0.05,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
ZTF J201946.97+334022.4 20260408.3374 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
Gaia DR3 1836281763839484032,2461138.8374,12.63,0.05,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 1836281763839484032 20260408.3374 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EM Cyg,2461138.8374,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EM Cyg 20260408.3374 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201841.02+310129.8,2461138.8374,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201841.02+310129.8 20260408.3374 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195934.90+285911.3,2461138.8374,13.48,0.05,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
ASASSN-V J195934.90+285911.3 20260408.3374 13.48CV 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
ASASSN-V J200234.18+270852.5,2461138.8374,12.99,0.05,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 J200234.18+270852.5 20260408.3374 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
NSVS 8366631,2461138.8374,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8366631 20260408.3374 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200100.12+324221.6,2461138.8374,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200100.12+324221.6 20260408.3374 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194253.72+255058.9,2461138.8374,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194253.72+255058.9 20260408.3374 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2029486126013515264,2461138.8374,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2029486126013515264 20260408.3374 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193813.04+294606.1,2461138.8374,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193813.04+294606.1 20260408.3374 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[WM2007] 1262,2461138.8374,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
[WM2007] 1262 20260408.3374 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201913.34+321540.3,2461138.8374,12.22,0.05,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
ASASSN-V J201913.34+321540.3 20260408.3374 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
NSVS 8404514,2461138.8374,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8404514 20260408.3374 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.8374,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.3374 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.8374,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.3374 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1955446+260450,2461138.8374,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1955446+260450 20260408.3374 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1837245107817975936,2461138.8374,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1837245107817975936 20260408.3374 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195912.62+300517.9,2461138.8374,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195912.62+300517.9 20260408.3374 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8545642,2461138.8374,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8545642 20260408.3374 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195338.96+262118.2,2461138.8374,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195338.96+262118.2 20260408.3374 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028545665632832512,2461138.8374,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028545665632832512 20260408.3374 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.1420+28.3682,2461138.8374,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.1420+28.3682 20260408.3374 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030799728851878528,2461138.8374,13.07,0.05,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
Gaia DR3 2030799728851878528 20260408.3374 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201456.38+273020.9,2461138.8374,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201456.38+273020.9 20260408.3374 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FY Cyg,2461138.8374,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FY Cyg 20260408.3374 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461138.83778028 08.04.2026 08:06:14.216 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23531
Objects passed selection criteria: 23505
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 21263
Average stars matched: 20699.5 (97.3499 %)
Memory usage VmPeak: 129064 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 Wed Apr 8 03:09:46 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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461138.83778028 08.04.2026 08:06:14.216 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 380
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 121 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): 220037
Objects passed selection criteria: 219522
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 182089
Average stars matched: 175562 (96.4156 %)
Memory usage VmPeak: 2116840 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 Wed Apr 8 03:15:31 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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: 2461138.83710222
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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:46.444 +30:02:24.85
Angular distance between the image centers 0.0622 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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:44.045 +30:01:39.68
Angular distance between the image centers 0.0645 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 19:59:46.444 +30:02:24.85
Second-epoch second image center 19:59:44.045 +30:01:39.68
Angular distance between the image centers 0.01524 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.hHRdaTTZOi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.pTTPH2W3zd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits &> /tmp/tmp.Ze0RRINaM7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits &> /tmp/tmp.zm55mdQfcQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 30878 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2644 to 309.4609 deg, Dec +24.2020 to +35.3348 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 290.2644 to 309.4609 deg, Dec 24.2020 to 35.3348 deg
Loaded 30795 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): 6699 out of 7455 total matches.
Matched with Tycho-2 7455 out of 30878 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854269
a=0.000000 b=1.000000 c=22.854269
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
3.0 pix fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
3.0 pix fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Limiting magnitude estimates:
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
14.2 mag. fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
14.2 mag. fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.5 (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.hHRdaTTZOi (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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3756, passed=30878
Got 30878 stars (including 27089 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 30878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 571 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 700 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: 641 matched stars entering correct_measured_positions(), 569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.90"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 631 matched stars entering correct_measured_positions(), 19509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.54"
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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 701 matched stars entering correct_measured_positions(), 19538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.51"
WARNING: Accuracy estimation diagnostic: 698 matched stars entering correct_measured_positions(), 21385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.18"
Excluding outliers - 698 stars left (next iteration limit 694)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.pTTPH2W3zd (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/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3771, passed=30931
Got 30931 stars (including 27121 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 30931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 610 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: 541 matched stars entering correct_measured_positions(), 474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.80"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 533 matched stars entering correct_measured_positions(), 15522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.95"
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 571 to 628 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 585 matched stars entering correct_measured_positions(), 15534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.91"
WARNING: Accuracy estimation diagnostic: 583 matched stars entering correct_measured_positions(), 16703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.33"
Excluding outliers - 583 stars left (next iteration limit 586)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.Ze0RRINaM7 (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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1608, passed=20002
Got 20002 stars (including 18384 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 20002 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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 19330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 19331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
WARNING: Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 19330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.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.zm55mdQfcQ (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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1637, passed=19987
Got 19987 stars (including 18340 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 19987 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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 938 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: 928 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 19435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits'
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52142.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51983_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 51983_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:32:11.36 +27:37:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52031_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52031_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:38.30 +27:55:35.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 52060_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52060_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:29.16 +31:26:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52062_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52062_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:02:12.00 +29:13:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52084_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52084_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:28.86 +30:29:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52113_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52113_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:03.08 +31:42:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52119_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52119_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:36:28.51 +29:24:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52126_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52126_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:36:26.26 +31:45:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52130_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52130_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:28.48 +27:01:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.590 2025283723876599680 292.86788379001 +27.03132272152 11.0043 9.7361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52132_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52132_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:57.49 +30:29:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52134_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52134_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:53.69 +31:12:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52142_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 52142_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:36.50 +31:51:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.152 2045073760606995840 292.65273694779 +31.86072181574 11.8970 11.5903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09276_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 09276_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:52.29 +28:19:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09275_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 09275_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:58.01 +28:30:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12059_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 12059_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:15:06.07 +29:45:47.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:46.444 +30:02:24.85
Angular distance between the image centers 0.0622 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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:44.045 +30:01:39.68
Angular distance between the image centers 0.0645 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 19:59:46.444 +30:02:24.85
Second-epoch second image center 19:59:44.045 +30:01:39.68
Angular distance between the image centers 0.01524 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.IsoHxDqypl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.EshHh5qrRV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits &> /tmp/tmp.xfkreJKtwj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits &> /tmp/tmp.QUZbrbk6nE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 281578 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2219 to 309.4679 deg, Dec +24.1963 to +35.3349 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 290.2219 to 309.4679 deg, Dec 24.1963 to 35.3349 deg
Loaded 30877 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): 5684 out of 8842 total matches.
Matched with Tycho-2 8842 out of 281578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629178
a=0.000000 b=1.000000 c=22.629178
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 265 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
2.9 pix fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
2.9 pix fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Limiting magnitude estimates:
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
14.2 mag. fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
14.2 mag. fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (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.IsoHxDqypl (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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=51531, passed=281520
Got 281520 stars (including 229582 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 281520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 692 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: 642 matched stars entering correct_measured_positions(), 589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.01"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 635 matched stars entering correct_measured_positions(), 211069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 754 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 715 matched stars entering correct_measured_positions(), 211109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
WARNING: Accuracy estimation diagnostic: 713 matched stars entering correct_measured_positions(), 228657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Excluding outliers - 713 stars left (next iteration limit 698)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.EshHh5qrRV (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/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=51082, passed=280646
Got 280646 stars (including 229187 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 280646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 584 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: 520 matched stars entering correct_measured_positions(), 457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.56"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 517 matched stars entering correct_measured_positions(), 153986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
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 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 154010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
WARNING: Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 174936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 567 stars left (next iteration limit 568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.xfkreJKtwj (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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=4, blended=20498, passed=134372
Got 134372 stars (including 113760 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 134372 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 945 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: 938 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 131054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 131052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 130977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.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.QUZbrbk6nE (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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=20872, passed=135707
Got 135707 stars (including 114725 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 135707 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 945 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: 937 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 132134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 132133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 132132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-05-15_20.00sec_-5.00C_LIGHT_0159.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.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_2026-04-08_CI_Cyg-08-Q2b1x1_030650_TTUQ2b1x1_633_gPqyxInD/wcs_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160.fits
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out103097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out230960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out230643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315961.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out315987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33042.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out43550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47986.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out54677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96873.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
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: 30s
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Considering the candidate 315806_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315806_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:02.96 +30:22:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315807_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315807_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:59:47.38 +30:32:47.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 315814_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315814_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:17:38.74 +33:19:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315815_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315815_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:13:13.60 +29:12:38.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 315817_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315817_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:04.50 +25:29:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.838 2024435858633802752 292.76799221572 +25.48603083885 13.0662 12.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315819_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315819_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:14:48.89 +32:44:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 315821_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315821_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:03:49.14 +31:03:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 315824_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315824_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:42.87 +26:29:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.639 2027785009725858304 297.17877679310 +26.49514880247 13.5909 12.9853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:18:28.68 +31:19:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315832_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315832_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:08:42.33 +32:53:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315833_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315833_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:17:41.74 +29:35:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.726 1861402168555752064 304.42208777630 +29.58610754021 13.0171 12.1717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315838_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315838_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:52.40 +33:10:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.571 2034947022328368768 296.46841674291 +33.17496229794 13.6111 12.8167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315848_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315848_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:25.99 +29:27:03.9 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 315854_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315854_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:18:52.60 +29:20:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 315859_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315859_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:09:26.63 +29:00:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 315868_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315868_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:25.97 +32:31:26.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 315881_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315881_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:53.96 +31:54:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.037 2033265800329655168 295.22344399247 +31.90544712185 13.9773 13.5039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315884_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315884_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:46:40.76 +30:57:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.257 2032222157651661568 296.67024051869 +30.95648071023 13.5903 12.6910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315886_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315886_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:00.58 +30:11:00.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 315887_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315887_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:36.31 +31:15:27.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 315898_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315898_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:39:40.21 +30:40:39.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 315907_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315907_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:15:05.68 +26:04:23.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 315909_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315909_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:53:45.89 +29:52:16.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 315917_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315917_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:57:28.04 +30:27:51.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 315924_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315924_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:26.99 +32:43:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315926_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315926_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:07:00.22 +29:34:09.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 315931_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315931_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315937_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315937_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:55.75 +29:15:32.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 315938_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315938_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:13.38 +29:36:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.873 2028856380759147136 298.05713302007 +29.60410080761 13.5573 13.0730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315939_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315939_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:46:54.12 +32:09:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.148 2034607204521448960 296.72552942362 +32.16482089522 13.3945 12.6458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315941_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315941_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:49.99 +32:06:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315945_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315945_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:34.49 +31:30:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.037 2033146091003116160 295.14357813506 +31.50963590953 13.3425 12.5639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315946_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315946_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315952_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315952_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315954_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315954_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:28:14.65 +32:05:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.391 2045148256833058688 292.06033730994 +32.09668050429 13.7411 13.2155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315958_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315958_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:43.66 +33:18:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315961_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315961_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315962_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315962_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:05:01.29 +28:29:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315964_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315964_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:28.58 +30:02:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.340 2030232591349019008 299.61833882220 +30.04327567598 13.2904 12.5563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:37:45.35 +28:54:29.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 315973_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315973_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315976_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315976_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 315980_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315980_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:39:08.74 +33:31:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.892 2046980592972955904 294.78679021027 +33.52932673436 13.1424 12.2841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315983_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315983_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:14.65 +31:30:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.182 2033040778414498176 295.81129004522 +31.51667373558 12.9967 12.1026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315986_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315986_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:16.53 +29:50:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315987_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315987_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 315989_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315989_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:03:16.36 +33:40:05.4 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 315991_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315991_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:32.03 +28:39:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315993_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 315993_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:17:21.96 +30:21:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.277 1861520709656478464 304.34091119331 +30.35001212731 12.7706 12.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315998_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 315998_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 316001_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316001_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:18:44.05 +27:30:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.696 1836176206412396032 304.68430799158 +27.51064721272 12.4090 11.3910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316006_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316006_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:45.96 +31:12:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316054_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316054_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:39.83 +27:54:38.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 316108_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316108_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:29.08 +31:26:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316250_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316250_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:58.87 +29:47:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.021 2032570561050574080 293.49495113466 +29.78305062625 11.7574 10.4105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316253_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316253_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:32.88 +27:57:52.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 316292_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 316292_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 316326_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316326_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:12.73 +33:44:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316330_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316330_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:25.84 +33:53:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316341_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316341_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:37:25.53 +29:37:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316367_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316367_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:30.24 +33:37:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316389_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316389_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:29:32.73 +31:21:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316403_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316403_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:56:39.62 +30:58:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316432_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316432_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:35:18.47 +27:52:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316443_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316443_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:09.30 +26:59:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316451_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316451_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:51.16 +27:06:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316465_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316465_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:37:09.66 +28:28:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316478_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316478_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:39.65 +26:58:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316499_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316499_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:42.47 +33:25:47.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316505_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316505_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:00:02.29 +25:57:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316508_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316508_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:50.62 +28:27:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316511_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316511_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:59:05.29 +33:20:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316514_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316514_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:14:42.20 +26:25:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316516_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316516_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:44.68 +32:11:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316518_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316518_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:31.46 +31:59:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316528_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316528_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:10.30 +33:27:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316553_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316553_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:58.02 +31:18:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316555_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316555_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:36:35.32 +31:17:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316562_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316562_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:50:39.93 +27:25:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316568_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 316568_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 316575_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316575_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:50:29.21 +32:56:07.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316576_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316576_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:29.63 +31:16:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316583_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316583_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:12:01.17 +26:44:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316592_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316592_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:27.63 +31:42:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316602_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316602_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:32:07.18 +28:15:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316620_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316620_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:10.78 +33:43:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316621_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316621_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:49.15 +33:55:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316629_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316629_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:34.62 +32:24:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316631_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316631_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:12.06 +30:12:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316635_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316635_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:51:44.03 +31:09:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316649_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316649_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:26.95 +30:29:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316666_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316666_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:16:53.31 +27:02:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316668_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316668_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:35.91 +29:24:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316670_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 316670_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316672_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316672_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:20.13 +30:14:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316684_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316684_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:50.43 +32:41:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316686_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316686_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:03.61 +30:59:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316691_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316691_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:50:42.68 +33:15:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316694_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316694_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:53:22.79 +26:28:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316696_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316696_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:57.45 +28:27:25.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316707_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316707_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:54:58.22 +33:08:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316713_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316713_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:46:36.20 +30:02:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316718_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316718_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:40.41 +31:25:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316719_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316719_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:15.59 +29:29:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316728_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316728_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:31.58 +31:39:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316729_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316729_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:38.19 +32:44:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316734_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316734_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:41:43.15 +31:04:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.294 2032932850138263168 295.42845042033 +31.07679014955 13.1942 11.0312 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316735_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316735_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:16.39 +26:58:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316736_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316736_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:39:04.25 +30:03:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.172 2032449820928187776 294.76761519491 +30.05712267982 11.9194 10.3303 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316738_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316738_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:37.18 +29:22:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316740_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316740_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:49.92 +30:39:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316745_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316745_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:54.60 +28:20:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.027 2031291661589245696 295.97813182958 +28.34514367597 13.2895 12.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316751_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316751_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:23.93 +32:47:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.407 2045557790554289024 292.85104414391 +32.79176533109 13.5343 12.5283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316753_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316753_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:28:58.73 +32:32:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316771_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316771_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:52.31 +33:54:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316776_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316776_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:42:46.55 +27:36:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316779_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316779_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:15:26.05 +27:51:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316780_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316780_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:43:33.76 +28:39:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316785_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316785_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:23.44 +27:18:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316786_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316786_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:41.38 +33:47:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316796_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316796_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:53:18.65 +28:24:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316799_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 316799_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 316811_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316811_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:17:09.43 +25:53:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316813_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316813_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:00:49.78 +32:59:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316818_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316818_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:59.52 +27:56:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316823_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316823_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:07:35.16 +30:07:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316828_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316828_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:02:17.61 +32:30:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 316842_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316842_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:49.82 +28:58:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316847_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316847_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:10.32 +28:26:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316849_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316849_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:35:29.11 +27:06:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316862_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316862_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:44:39.86 +30:43:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316865_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316865_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:57:14.81 +31:41:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316871_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316871_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:05:18.22 +33:28:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316877_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316877_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:55.69 +29:30:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.903 2031657283564064256 295.23190141669 +29.50875310148 13.7486 12.8301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316890_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316890_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 316905_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316905_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:26.17 +32:01:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316906_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316906_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:44.20 +30:58:28.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316909_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316909_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:05.71 +33:52:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316910_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316910_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:48:13.23 +31:34:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.041 2033758656431613184 297.05349072955 +31.57721130556 11.5574 9.8655 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316932_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316932_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:01.75 +32:57:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.790 2035069617870105344 298.00641123636 +32.95697223049 13.6565 13.1877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316937_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316937_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:08.65 +29:40:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.569 2032411544176994688 294.53605251875 +29.68151889570 13.3490 10.8885 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:48.56 +30:54:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.917 2032774657895727744 293.45150430560 +30.91524937319 12.2726 10.4128 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316984_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 316984_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:35:51.26 +31:49:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317005_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317005_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:50:48.28 +31:56:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317011_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317011_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:46.68 +34:10:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317023_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317023_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:34:59.74 +25:54:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.386 2024554610236503040 293.74755067778 +25.90245214149 12.3997 10.8082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317055_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317055_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:05:57.77 +29:46:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317056_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317056_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:57:03.66 +30:46:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.173 2030505476401547392 299.26488652311 +30.76899067897 13.7261 13.1264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317059_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317059_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:51:28.73 +32:47:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317063_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317063_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:45:41.69 +33:15:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.959 2034994473130823040 296.42356575304 +33.25057152409 12.4877 11.0237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317069_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317069_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:50:20.33 +29:29:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317081_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317081_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:51:42.67 +30:11:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.365 2031891681356800384 297.92776475614 +30.18646168991 12.1827 10.5515 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317092_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317092_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:23.41 +31:25:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.631 2053844294287119104 304.84844891734 +31.43256318826 12.4441 10.8535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317102_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317102_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:51:11.92 +27:06:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.940 2027925231831457024 297.80007182818 +27.10448279666 13.2874 12.1664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317116_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317116_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:01.40 +33:11:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317120_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317120_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:04:35.45 +26:29:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317183_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 317183_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:04:54.27 +29:46:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.705 2029790965608949248 301.22632649729 +29.77011604778 12.8349 10.5909 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68822_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 68822_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:12:39.76 +28:05:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46374_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 46374_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:07:07.41 +27:06:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45642_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 45642_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 46954_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 46954_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 114440_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 114440_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:12:57.90 +29:38:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 313682_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 313682_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:02:12.86 +30:57:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 31831_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:14:35.10 +26:27:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108947_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 108947_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:35:26.89 +29:01:29.2 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 110658_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 110658_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:52:10.34 +29:21:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120106_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 120106_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:15:06.02 +29:45:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242260_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 242260_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:16.96 +33:44:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108492_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 108492_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:06:39.18 +29:24:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210789_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 210789_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 104878_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 104878_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:02:12.01 +29:13:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49137_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 49137_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:51:01.57 +27:04:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211187_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 211187_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 111422_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 111422_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:45.66 +29:24:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166201_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 166201_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:04:45.50 +31:12:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199052_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 199052_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 82746_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 82746_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 230643_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 230643_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 20441_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 20441_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 43550_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 43550_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 123987_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 123987_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 213964_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 213964_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 87644_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 87644_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:18:25.21 +28:44:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62278_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 62278_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 114707_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 114707_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 145467_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 145467_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 217695_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 217695_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:27.91 +32:53:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22807_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 22807_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 208479_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 208479_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:55:32.33 +32:33:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230960_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 230960_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:59:48.83 +33:23:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.938 2034399809139800064 299.95307280175 +33.38769426245 11.4110 9.8847 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124027_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 124027_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 101455_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 101455_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 103097_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 103097_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:41:18.12 +28:56:37.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 94562_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 94562_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 62764_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 62764_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 169183_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 169183_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:19:52.64 +31:20:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.637 2053828106543245312 304.96927514095 +31.33730882159 12.1708 10.8537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81792_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 81792_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 38958_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 38958_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 25199_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 25199_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:16:07.45 +26:07:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72014_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 72014_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 80945_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 80945_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:18:56.16 +28:32:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73692_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 73692_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:26.85 +28:05:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202882_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 202882_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 87433_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 87433_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 161186_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 161186_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:20:03.07 +31:04:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298383_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 298383_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:30:20.78 +30:54:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52510_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 52510_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 110408_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 110408_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 155851_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 155851_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:22.91 +30:49:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160448_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 160448_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:16:37.27 +31:01:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242176_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 242176_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 202270_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 202270_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 42746_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 42746_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:53:46.48 +26:49:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138011_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 138011_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 95893_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 95893_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:33.23 +28:33:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 246966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:44:25.05 +33:18:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243527_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 243527_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 62123_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 62123_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 154690_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 154690_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 159120_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 159120_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 96873_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 96873_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 189527_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 189527_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:09:43.56 +31:59:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119004_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 119004_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:58:14.01 +29:41:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 307955_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 307955_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:09:13.24 +29:29:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.670 2029545289166146048 302.30566757279 +29.48864758281 12.3605 10.7726 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 47986_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 47986_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 68455_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 68455_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 211071_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 211071_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 25667_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 25667_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 107506_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 107506_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 102097_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 102097_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:42:35.37 +28:56:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127236_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 127236_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:03:10.01 +29:59:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135520_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 135520_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:01:12.15 +30:12:20.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)
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Considering the candidate 53538_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 53538_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:31:51.14 +26:56:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130851_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 130851_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 296366_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 296366_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:49.63 +32:24:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.943 2045351322893213440 294.70611069229 +32.40238676132 12.1237 10.2182 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79479_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 79479_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 197262_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 197262_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 134579_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 134579_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:15:04.33 +30:14:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34870_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 34870_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 306420_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 306420_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:49:29.12 +26:21:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.222 2027034661758210176 297.37127245815 +26.36477934826 12.5664 11.0300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295549_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 295549_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 295444_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 295444_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:16:18.55 +28:48:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295172_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 295172_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 27245_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 27245_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 83979_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 83979_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 131640_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 131640_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 80414_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 80414_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 33042_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 33042_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 294877_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 294877_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 294841_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 294841_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 97966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 97966_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:38:58.05 +28:30:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294477_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 294477_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:59:15.39 +25:54:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.498 1835025773650679424 299.81542760966 +25.91568396866 12.5323 11.0892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236091_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 236091_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:57:07.79 +33:51:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124163_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 124163_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:40:31.65 +29:36:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175549_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 175549_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 186339_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 186339_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:20:28.70 +31:53:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.713 2054235754786768640 305.12014152482 +31.89723433114 11.7698 10.2515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170841_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 170841_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:20:18.26 +31:23:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54677_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 54677_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
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Considering the candidate 90024_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 90024_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:33:52.29 +28:19:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240308_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 240308_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:13:30.35 +33:47:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293989_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 293989_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 20:01:49.00 +26:31:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.726 1835164728751977216 300.45490956586 +26.52002630528 11.7630 10.2399 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43055_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 43055_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:47:37.12 +26:45:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198834_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
Preparing report for the candidate 198834_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109075_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160
The candidate 109075_fd_Cyg-08-Q2b1x1_2026-04-08_03-06-14_20.00sec_-4.90C_LIGHT_0160 did not pass the final checks
**** FOUND 19:29:15.86 +28:54:11.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 77s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:50:45.14 +29:02:22.4
20:11:37.27 +29:24:33.0
19:45:02.31 +29:15:01.3
20:09:10.08 +29:37:51.3
19:38:22.54 +29:33:33.9
20:02:29.70 +29:51:39.9
19:38:13.24 +29:46:09.6
19:59:12.57 +30:05:16.1
20:20:05.99 +30:21:21.9
19:52:14.37 +30:26:27.6
20:18:40.81 +31:01:28.2
20:05:09.33 +31:30:32.5
20:19:13.04 +32:15:39.1
19:45:10.69 +32:03:07.9
20:19:52.56 +32:19:20.9
20:20:31.46 +32:26:46.4
19:56:37.36 +32:22:10.8
20:18:23.72 +25:52:52.4
19:44:34.58 +32:29:11.4
20:01:00.29 +32:42:19.8
20:07:24.70 +32:45:12.3
20:13:33.19 +32:51:47.1
20:19:44.99 +26:00:33.7
20:05:23.74 +33:24:52.3
19:49:50.73 +33:33:35.6
20:19:46.59 +33:40:16.7
19:42:53.65 +25:51:01.8
19:55:44.68 +26:04:52.5
19:44:33.53 +28:22:33.1
19:53:13.81 +28:44:13.2
19:45:36.51 +29:34:51.1
20:18:02.72 +28:06:16.4
20:19:59.17 +33:20:56.1
20:16:14.35 +31:05:32.0
20:16:09.59 +25:47:09.2
20:01:11.89 +32:21:09.6
19:41:07.10 +28:21:33.4
19:34:47.19 +28:00:22.9
20:04:42.75 +33:54:04.8
19:37:05.92 +28:11:51.7
19:34:07.17 +30:13:32.1
19:28:47.92 +30:54:15.7
20:11:30.99 +29:09:18.4
19:53:39.08 +26:21:21.0
19:59:29.28 +26:30:06.6
20:19:46.86 +26:48:07.4
19:30:11.28 +26:28:05.6
19:56:37.69 +26:58:42.1
19:57:24.62 +27:03:18.8
20:02:34.21 +27:08:54.1
20:14:11.14 +27:24:59.9
20:14:55.94 +27:30:23.6
20:20:07.44 +27:50:25.3
20:17:19.27 +27:50:07.5
20:17:12.73 +27:51:51.0
19:32:09.06 +27:33:42.6
20:02:06.69 +28:09:42.5
19:36:32.82 +28:04:04.2
20:19:25.03 +28:31:43.0
20:15:46.39 +28:34:06.9
19:44:12.00 +28:19:21.0
20:12:46.18 +28:38:07.1
20:07:20.85 +28:43:43.1
20:19:23.04 +28:59:32.6
19:59:34.98 +28:59:12.5
########### Completed Cyg-08-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 ####
20:19:59.17 +33:20:56.1
20:16:14.35 +31:05:32.0
20:16:09.59 +25:47:09.2
20:01:11.89 +32:21:09.6
19:41:07.10 +28:21:33.4
19:34:47.19 +28:00:22.9
20:04:42.75 +33:54:04.8
19:37:05.92 +28:11:51.7
19:34:07.17 +30:13:32.1
19:28:47.92 +30:54:15.7
20:11:30.99 +29:09:18.4
19:56:37.69 +26:58:42.1
19:57:24.62 +27:03:18.8
19:44:34.58 +32:29:11.4
20:07:24.70 +32:45:12.3
20:19:52.56 +32:19:20.9
19:44:12.00 +28:19:21.0
20:05:23.74 +33:24:52.3
20:18:23.72 +25:52:52.4
19:30:11.28 +26:28:05.6
19:38:22.54 +29:33:33.9
20:13:33.19 +32:51:47.1
20:17:19.27 +27:50:07.5
20:09:10.08 +29:37:51.3
19:52:14.37 +30:26:27.6
20:19:44.99 +26:00:33.7
20:02:29.70 +29:51:39.9
19:50:45.14 +29:02:22.4
20:19:23.04 +28:59:32.6
20:17:12.73 +27:51:51.0
20:15:46.39 +28:34:06.9
20:19:46.86 +26:48:07.4
20:02:06.69 +28:09:42.5
19:56:37.36 +32:22:10.8
20:07:20.85 +28:43:43.1
20:14:11.14 +27:24:59.9
19:45:02.31 +29:15:01.3
19:49:50.73 +33:33:35.6
20:20:31.46 +32:26:46.4
20:20:05.99 +30:21:21.9
20:19:46.59 +33:40:16.7
20:20:07.44 +27:50:25.3
19:38:40.05 +30:30:29.1
20:18:40.81 +31:01:28.2
19:59:34.98 +28:59:12.5
20:02:34.21 +27:08:54.1
19:32:09.06 +27:33:42.6
20:01:00.29 +32:42:19.8
19:42:53.65 +25:51:01.8
20:11:37.27 +29:24:33.0
19:38:13.24 +29:46:09.6
19:36:32.82 +28:04:04.2
20:19:13.04 +32:15:39.1
19:59:29.28 +26:30:06.6
20:18:02.72 +28:06:16.4
19:45:36.51 +29:34:51.1
19:55:44.68 +26:04:52.5
20:12:46.18 +28:38:07.1
19:59:12.57 +30:05:16.1
20:19:25.03 +28:31:43.0
19:53:39.08 +26:21:21.0
19:53:13.81 +28:44:13.2
19:44:33.53 +28:22:33.1
20:05:09.33 +31:30:32.5
20:14:55.94 +27:30:23.6
19:45:10.69 +32:03:07.9
###################################################################################
20:19:59.17 +33:20:56.1 -- not an asteroid (will add it to exclusion list)
20:16:14.35 +31:05:32.0 -- not an asteroid (will add it to exclusion list)
20:16:09.59 +25:47:09.2 -- not an asteroid (will add it to exclusion list)
20:01:11.89 +32:21:09.6 -- not an asteroid (will add it to exclusion list)
19:41:07.10 +28:21:33.4 -- not an asteroid (will add it to exclusion list)
19:34:47.19 +28:00:22.9 -- not an asteroid (will add it to exclusion list)
20:04:42.75 +33:54:04.8 -- not an asteroid (will add it to exclusion list)
19:37:05.92 +28:11:51.7 -- not an asteroid (will add it to exclusion list)
19:34:07.17 +30:13:32.1 -- not an asteroid (will add it to exclusion list)
19:28:47.92 +30:54:15.7 -- not an asteroid (will add it to exclusion list)
20:11:30.99 +29:09:18.4 -- not an asteroid (will add it to exclusion list)
19:56:37.69 +26:58:42.1 -- not an asteroid (will add it to exclusion list)
19:57:24.62 +27:03:18.8 -- not an asteroid (will add it to exclusion list)
19:44:34.58 +32:29:11.4 -- not an asteroid (will add it to exclusion list)
20:07:24.70 +32:45:12.3 -- not an asteroid (will add it to exclusion list)
20:19:52.56 +32:19:20.9 -- not an asteroid (will add it to exclusion list)
19:44:12.00 +28:19:21.0 -- not an asteroid (will add it to exclusion list)
20:05:23.74 +33:24:52.3 -- not an asteroid (will add it to exclusion list)
20:18:23.72 +25:52:52.4 -- not an asteroid (will add it to exclusion list)
19:30:11.28 +26:28:05.6 -- not an asteroid (will add it to exclusion list)
19:38:22.54 +29:33:33.9 -- not an asteroid (will add it to exclusion list)
20:13:33.19 +32:51:47.1 -- not an asteroid (will add it to exclusion list)
20:17:19.27 +27:50:07.5 -- not an asteroid (will add it to exclusion list)
20:09:10.08 +29:37:51.3 -- not an asteroid (will add it to exclusion list)
19:52:14.37 +30:26:27.6 -- not an asteroid (will add it to exclusion list)
20:19:44.99 +26:00:33.7 -- not an asteroid (will add it to exclusion list)
20:02:29.70 +29:51:39.9 -- not an asteroid (will add it to exclusion list)
19:50:45.14 +29:02:22.4 -- not an asteroid (will add it to exclusion list)
20:19:23.04 +28:59:32.6 -- not an asteroid (will add it to exclusion list)
20:17:12.73 +27:51:51.0 -- not an asteroid (will add it to exclusion list)
20:15:46.39 +28:34:06.9 -- not an asteroid (will add it to exclusion list)
20:19:46.86 +26:48:07.4 -- not an asteroid (will add it to exclusion list)
20:02:06.69 +28:09:42.5 -- not an asteroid (will add it to exclusion list)
19:56:37.36 +32:22:10.8 -- not an asteroid (will add it to exclusion list)
20:07:20.85 +28:43:43.1 -- not an asteroid (will add it to exclusion list)
20:14:11.14 +27:24:59.9 -- not an asteroid (will add it to exclusion list)
19:45:02.31 +29:15:01.3 -- not an asteroid (will add it to exclusion list)
19:49:50.73 +33:33:35.6 -- not an asteroid (will add it to exclusion list)
20:20:31.46 +32:26:46.4 -- not an asteroid (will add it to exclusion list)
20:20:05.99 +30:21:21.9 -- not an asteroid (will add it to exclusion list)
20:19:46.59 +33:40:16.7 -- not an asteroid (will add it to exclusion list)
20:20:07.44 +27:50:25.3 -- not an asteroid (will add it to exclusion list)
19:38:40.05 +30:30:29.1 -- listed in neverexclude_list.txt (will NOT add it to exclusion list)
20:18:40.81 +31:01:28.2 -- not an asteroid (will add it to exclusion list)
19:59:34.98 +28:59:12.5 -- not an asteroid (will add it to exclusion list)
20:02:34.21 +27:08:54.1 -- not an asteroid (will add it to exclusion list)
19:32:09.06 +27:33:42.6 -- not an asteroid (will add it to exclusion list)
20:01:00.29 +32:42:19.8 -- not an asteroid (will add it to exclusion list)
19:42:53.65 +25:51:01.8 -- not an asteroid (will add it to exclusion list)
20:11:37.27 +29:24:33.0 -- not an asteroid (will add it to exclusion list)
19:38:13.24 +29:46:09.6 -- not an asteroid (will add it to exclusion list)
19:36:32.82 +28:04:04.2 -- not an asteroid (will add it to exclusion list)
20:19:13.04 +32:15:39.1 -- not an asteroid (will add it to exclusion list)
19:59:29.28 +26:30:06.6 -- not an asteroid (will add it to exclusion list)
20:18:02.72 +28:06:16.4 -- not an asteroid (will add it to exclusion list)
19:45:36.51 +29:34:51.1 -- not an asteroid (will add it to exclusion list)
19:55:44.68 +26:04:52.5 -- not an asteroid (will add it to exclusion list)
20:12:46.18 +28:38:07.1 -- not an asteroid (will add it to exclusion list)
19:59:12.57 +30:05:16.1 -- not an asteroid (will add it to exclusion list)
20:19:25.03 +28:31:43.0 -- not an asteroid (will add it to exclusion list)
19:53:39.08 +26:21:21.0 -- not an asteroid (will add it to exclusion list)
19:53:13.81 +28:44:13.2 -- not an asteroid (will add it to exclusion list)
19:44:33.53 +28:22:33.1 -- not an asteroid (will add it to exclusion list)
20:05:09.33 +31:30:32.5 -- not an asteroid (will add it to exclusion list)
20:14:55.94 +27:30:23.6 -- not an asteroid (will add it to exclusion list)
19:45:10.69 +32:03:07.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:28:47.92 +30:54:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:11.28 +26:28:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:09.06 +27:33:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:07.17 +30:13:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:47.19 +28:00:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:32.82 +28:04:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:05.92 +28:11:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:13.24 +29:46:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:22.54 +29:33:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:07.10 +28:21:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:53.65 +25:51:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:12.00 +28:19:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:33.53 +28:22:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:34.58 +32:29:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:02.31 +29:15:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:10.69 +32:03:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:36.51 +29:34:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:50.73 +33:33:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:45.14 +29:02:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:14.37 +30:26:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:13.81 +28:44:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:39.08 +26:21:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:44.68 +26:04:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:37.36 +32:22:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:37.69 +26:58:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:24.62 +27:03:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:12.57 +30:05:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:29.28 +26:30:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:34.98 +28:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:00.29 +32:42:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:11.89 +32:21:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:06.69 +28:09:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:29.70 +29:51:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:34.21 +27:08:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:42.75 +33:54:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:09.33 +31:30:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:23.74 +33:24:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:20.85 +28:43:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:24.70 +32:45:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:10.08 +29:37:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:30.99 +29:09:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:37.27 +29:24:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:46.18 +28:38:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:33.19 +32:51:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:11.14 +27:24:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:55.94 +27:30:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:46.39 +28:34:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:09.59 +25:47:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:14.35 +31:05:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:12.73 +27:51:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:19.27 +27:50:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:02.72 +28:06:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:23.72 +25:52:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:40.81 +31:01:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:13.04 +32:15:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:23.04 +28:59:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:25.03 +28:31:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:44.99 +26:00:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:46.59 +33:40:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:46.86 +26:48:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:52.56 +32:19:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:59.17 +33:20:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:05.99 +30:21:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:07.44 +27:50:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:31.46 +32:26:46.4 -- 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)
19:28:47.92 +30:54:15.7 -- a known variable star
19:30:11.28 +26:28:05.6 -- a known variable star
19:32:09.06 +27:33:42.6 -- a known variable star
19:34:07.17 +30:13:32.1 -- not a known variable star
19:34:47.19 +28:00:22.9 -- not a known variable star
19:36:32.82 +28:04:04.2 -- a known variable star
19:37:05.92 +28:11:51.7 -- a known variable star
19:38:13.24 +29:46:09.6 -- a known variable star
19:38:22.54 +29:33:33.9 -- a known variable star
19:41:07.10 +28:21:33.4 -- a known variable star
19:42:53.65 +25:51:01.8 -- a known variable star
19:44:12.00 +28:19:21.0 -- a known variable star
19:44:33.53 +28:22:33.1 -- not a known variable star
19:44:34.58 +32:29:11.4 -- a known variable star
19:45:02.31 +29:15:01.3 -- a known variable star
19:45:10.69 +32:03:07.9 -- a known variable star
19:45:36.51 +29:34:51.1 -- not a known variable star
19:49:50.73 +33:33:35.6 -- a known variable star
19:50:45.14 +29:02:22.4 -- a known variable star
19:52:14.37 +30:26:27.6 -- a known variable star
19:53:13.81 +28:44:13.2 -- a known variable star
19:53:39.08 +26:21:21.0 -- a known variable star
19:55:44.68 +26:04:52.5 -- a known variable star
19:56:37.36 +32:22:10.8 -- a known variable star
19:56:37.69 +26:58:42.1 -- a known variable star
19:57:24.62 +27:03:18.8 -- a known variable star
19:59:12.57 +30:05:16.1 -- a known variable star
19:59:29.28 +26:30:06.6 -- a known variable star
19:59:34.98 +28:59:12.5 -- a known variable star
20:01:00.29 +32:42:19.8 -- a known variable star
20:01:11.89 +32:21:09.6 -- a known variable star
20:02:06.69 +28:09:42.5 -- a known variable star
20:02:29.70 +29:51:39.9 -- a known variable star
20:02:34.21 +27:08:54.1 -- a known variable star
20:04:42.75 +33:54:04.8 -- a known variable star
20:05:09.33 +31:30:32.5 -- not a known variable star
20:05:23.74 +33:24:52.3 -- not a known variable star
20:07:20.85 +28:43:43.1 -- a known variable star
20:07:24.70 +32:45:12.3 -- a known variable star
20:09:10.08 +29:37:51.3 -- a known variable star
20:11:30.99 +29:09:18.4 -- a known variable star
20:11:37.27 +29:24:33.0 -- a known variable star
20:12:46.18 +28:38:07.1 -- a known variable star
20:13:33.19 +32:51:47.1 -- a known variable star
20:14:11.14 +27:24:59.9 -- a known variable star
20:14:55.94 +27:30:23.6 -- a known variable star
20:15:46.39 +28:34:06.9 -- a known variable star
20:16:09.59 +25:47:09.2 -- a known variable star
20:16:14.35 +31:05:32.0 -- not a known variable star
20:17:12.73 +27:51:51.0 -- a known variable star
20:17:19.27 +27:50:07.5 -- a known variable star
20:18:02.72 +28:06:16.4 -- not a known variable star
20:18:23.72 +25:52:52.4 -- not a known variable star
20:18:40.81 +31:01:28.2 -- a known variable star
20:19:13.04 +32:15:39.1 -- a known variable star
20:19:23.04 +28:59:32.6 -- a known variable star
20:19:25.03 +28:31:43.0 -- a known variable star
20:19:44.99 +26:00:33.7 -- not a known variable star
20:19:46.59 +33:40:16.7 -- a known variable star
20:19:46.86 +26:48:07.4 -- a known variable star
20:19:52.56 +32:19:20.9 -- a known variable star
20:19:59.17 +33:20:56.1 -- not a known variable star
20:20:05.99 +30:21:21.9 -- not a known variable star
20:20:07.44 +27:50:25.3 -- a known variable star
20:20:31.46 +32:26:46.4 -- a known variable star
Found 12 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
65 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 65 (excluding asteroids and hot pixels, 12 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461138.83710222 -observatory V36
23:29:44.56 -05:39:45.6 Mercury (0.3mag)
02:31:40.37 +14:46:44.4 Venus (-3.9mag)
23:56:01.99 -01:32:13.7 Mars (1.2mag)
07:09:28.09 +22:51:16.1 Jupiter (-2.2mag)
00:25:44.13 +00:27:22.4 Saturn (0.9mag)
03:46:08.26 +19:42:26.6 Uranus (5.8mag)
00:09:49.24 -00:21:49.4 Neptune (7.8mag)
20:33:21.90 -22:52:27.3 Pluto (14.5mag)
17:52:14.03 -28:54:39.3 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 03:09 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461138.83710222:
07:09:22.29 +22:51:25.4 Io (5.7mag)
07:09:19.53 +22:51:35.7 Europa (5.9mag)
07:09:48.51 +22:50:34.8 Ganymede (5.3mag)
07:08:53.37 +22:52:25.6 Callisto (6.5mag)
07:13:06.70 +22:42:39.0 Himalia (15.3mag)
07:09:29.68 +22:51:14.9 Thebe (16.2mag)
07:13:07.53 +23:11:51.5 Elara (17.3mag)
07:07:49.68 +23:35:16.9 Pasiphae (17.4mag)
07:17:57.45 +22:48:27.8 Carme (18.4mag)
00:25:47.49 +00:27:12.6 Titan (8.8mag)
00:25:49.57 +00:27:23.1 Rhea (10.1mag)
00:25:39.80 +00:28:40.3 Iapetus (11.5mag)
00:25:53.21 +00:27:07.8 Hyperion (14.8mag)
00:27:26.85 +00:36:58.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 03:09 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.83710222:
14:59:13.15 -10:16:11.7 JWST
14:38:33.76 +56:06:31.9 Chandra
08:27:44.72 -46:16:24.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 03:09 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.83710222 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:20.77 -28:20:56.5 13.9mag P/2010 H2 (Vales)
05:01:28.01 -70:02:15.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:56.08 +31:23:18.1 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.01 +09:37:48.3 17.6mag C/2021 G2 (ATLAS)
23:08:01.66 +28:56:29.6 17.0mag C/2022 E2 (ATLAS)
04:20:24.98 +25:49:31.6 15.9mag C/2022 N2 (PANSTARRS)
09:02:06.22 +31:56:26.8 16.2mag C/2022 QE78 (ATLAS)
08:30:08.79 -00:59:21.2 17.3mag C/2022 R6 (PANSTARRS)
18:55:16.11 +17:52:48.8 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:57.32 -11:37:52.9 17.6mag P/2023 B1 (PANSTARRS)
09:11:34.57 -13:08:25.5 17.6mag C/2023 F3 (ATLAS)
21:45:59.30 +62:28:51.5 17.5mag C/2023 H5 (Lemmon)
19:25:03.42 -03:37:46.2 14.2mag C/2023 R1 (PANSTARRS)
21:41:48.60 +84:52:58.5 17.8mag C/2023 X2 (Lemmon)
06:15:02.30 +63:33:47.8 17.1mag C/2024 A1 (ATLAS)
04:56:09.46 +15:28:21.2 10.5mag C/2024 E1 (Wierzchos)
16:23:55.13 +05:07:50.5 17.4mag C/2024 G6 (ATLAS)
20:18:21.28 +13:14:12.0 14.7mag C/2024 J3 (ATLAS)
03:19:36.54 -23:34:42.6 16.4mag C/2024 T5 (ATLAS)
05:10:23.63 +47:15:26.4 17.7mag C/2025 J1 (Borisov)
14:10:30.03 +39:28:20.8 14.9mag C/2025 L1 (ATLAS)
03:13:31.28 -25:03:25.0 17.8mag C/2025 Q3 (ATLAS)
22:59:52.40 +19:48:23.3 9.7mag C/2025 R3 (PANSTARRS)
12:57:27.36 +02:31:54.9 17.5mag C/2025 Y1 (ATLAS)
02:05:46.66 +03:57:18.5 9.7mag C/2026 A1 (MAPS)
23:37:16.79 +35:42:31.7 14.3mag C/2026 B2 (Sun-Gao)
18:27:59.23 -10:06:55.1 12.3mag 10P/Tempel
15:10:18.66 +03:56:09.6 13.3mag 24P/Schaumasse
11:05:03.57 -01:47:10.9 15.7mag 29P/Schwassmann-Wachmann
17:57:55.82 -09:54:22.3 17.8mag 40P/Vaisala
10:38:25.44 -04:45:00.9 16.8mag 43P/Wolf-Harrington
01:36:50.93 +16:10:10.9 17.2mag 47P/Ashbrook-Jackson
06:57:00.62 +38:38:06.2 17.0mag 63P/Wild
23:19:08.57 -12:23:13.2 15.7mag 65P/Gunn
03:43:09.20 +18:32:00.5 15.9mag 76P/West-Kohoutek-Ikemura
00:48:44.81 +06:42:46.1 14.4mag 78P/Gehrels
22:39:21.20 -11:38:50.1 14.5mag 88P/Howell
01:49:01.76 +18:33:02.7 15.1mag 93P/Lovas
04:40:43.18 +31:51:24.2 16.3mag 123P/West-Hartley
08:19:59.20 +41:53:58.3 16.2mag 124P/Mrkos
02:21:28.07 +13:30:13.5 16.4mag 128P/Shoemaker-Holt
02:32:33.92 +13:31:57.4 17.5mag 131P/Mueller
00:46:37.87 +10:26:30.0 11.1mag 141P/Machholz
00:56:26.46 +01:59:51.1 11.1mag 141P-A/Machholz
23:45:45.86 -01:44:46.0 13.8mag 141P-D/Machholz
01:25:53.75 +03:41:42.6 17.9mag 141P-I/Machholz
00:41:04.77 -05:21:26.6 15.2mag 162P/SidingSpring
10:30:19.32 +31:22:28.2 17.9mag 164P/Christensen
06:22:21.54 +24:28:14.8 17.9mag 198P/ODAS
15:04:59.17 -00:55:46.9 17.4mag 210P/Christensen
21:15:45.33 -13:18:12.0 17.5mag 218P/LINEAR
17:13:44.72 -14:49:56.8 16.2mag 235P/LINEAR
05:18:08.51 +34:03:31.1 16.6mag 240P/NEAT
07:35:02.27 -06:01:53.0 17.6mag 242P/Spahr
15:45:19.17 +06:27:49.9 17.5mag 391P/Kowalski
07:31:32.46 +21:19:40.6 17.6mag 450P/LONEOS
05:24:53.92 +45:28:59.9 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 03:09 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 8 03:09 asassn_transients_list.txt
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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 8 03:09 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:46:09.818 -61:19:51.60 AT 2026icy 2026-04-02.36 18.325
15:30:09.406 +58:57:13.42 AT 2026icx 2026-03-30.43 19.684
11:28:54.874 +21:06:30.69 AT 2026icw 2026-04-02.30 19.2031
12:10:50.697 +66:55:30.99 SN 2026icv 2026-04-02.28 18.5118
07:36:32.513 +50:19:24.81 AT 2026icu 2026-04-02.24 19.2237
08:38:37.560 +02:03:38.03 AT 2026ict 2026-04-02.15 19.0837
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
-rw-r--r-- 1 apache apache 30K Apr 8 03:09 tns_transients_list.txt
