This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk
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
V0702 Cyg,2461138.8362,8.52,0.05,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
V0702 Cyg 20260408.3362 8.52CV 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 3275927,2461138.8362,9.33,0.05,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
NSVS 3275927 20260408.3362 9.33CV 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
ATO J323.2075+54.2841,2461138.8362,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.2075+54.2841 20260408.3362 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9032+55.9641,2461138.8362,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9032+55.9641 20260408.3362 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212633.35+515524.6,2461138.8362,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212633.35+515524.6 20260408.3362 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212848.12+505838.6,2461138.8362,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212848.12+505838.6 20260408.3362 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.3614+51.9715,2461138.8362,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.3614+51.9715 20260408.3362 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165866245470446592,2461138.8362,13.07,0.05,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 2165866245470446592 20260408.3362 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 J212614.99+500704.4,2461138.8362,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212614.99+500704.4 20260408.3362 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213619.01+511346.1,2461138.8362,13.12,0.05,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
ASASSN-V J213619.01+511346.1 20260408.3362 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
ATO J316.4504+49.9594,2461138.8362,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.4504+49.9594 20260408.3362 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8362,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3362 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213124.42+503250.1,2461138.8362,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213124.42+503250.1 20260408.3362 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V3082 Cyg,2461138.8362,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3082 Cyg 20260408.3362 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J319.5489+49.7807,2461138.8362,13.11,0.05,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
ATO J319.5489+49.7807 20260408.3362 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
ASASSN-V J212748.43+520106.9,2461138.8362,12.35,0.05,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
ASASSN-V J212748.43+520106.9 20260408.3362 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
NSVS 3272338,2461138.8362,12.26,0.05,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
NSVS 3272338 20260408.3362 12.26CV 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
Gaia DR3 2165924970565928832,2461138.8362,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165924970565928832 20260408.3362 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V3158 Cyg,2461138.8362,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3158 Cyg 20260408.3362 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GL Cep,2461138.8362,10.04,0.05,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
GL Cep 20260408.3362 10.04CV 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 3284223,2461138.8362,12.24,0.05,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
NSVS 3284223 20260408.3362 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
ASASSN-V J213315.06+504740.2,2461138.8362,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213315.06+504740.2 20260408.3362 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213153.92+512948.2,2461138.8362,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213153.92+512948.2 20260408.3362 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212523.17+550902.6,2461138.8362,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212523.17+550902.6 20260408.3362 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213234.19+515051.8,2461138.8362,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213234.19+515051.8 20260408.3362 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2170173002450411136,2461138.8362,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2170173002450411136 20260408.3362 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
V2060 Cyg,2461138.8362,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2060 Cyg 20260408.3362 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J205226.54+531202.9,2461138.8362,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205226.54+531202.9 20260408.3362 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211641.86+571041.7,2461138.8362,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211641.86+571041.7 20260408.3362 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7679+52.0745,2461138.8362,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.7679+52.0745 20260408.3362 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8362,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3362 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212241.65+543814.5,2461138.8362,13.11,0.05,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 J212241.65+543814.5 20260408.3362 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
NSVS 5858708,2461138.8362,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5858708 20260408.3362 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.7759+51.4759,2461138.8362,13.11,0.05,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
ATO J323.7759+51.4759 20260408.3362 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
V3126 Cyg,2461138.8362,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3126 Cyg 20260408.3362 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8362,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3362 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212318.35+494725.0,2461138.8362,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212318.35+494725.0 20260408.3362 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 2171137407292873216,2461138.8362,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171137407292873216 20260408.3362 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2174452022533671808,2461138.8362,12.96,0.05,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
Gaia DR3 2174452022533671808 20260408.3362 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
NSVS 3261260,2461138.8362,12.02,0.05,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
NSVS 3261260 20260408.3362 12.02CV 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
Gaia DR3 2171593017419529600,2461138.8362,13.05,0.05,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 2171593017419529600 20260408.3362 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 J212325.26+534359.5,2461138.8362,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212325.26+534359.5 20260408.3362 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2050059+560817,2461138.8362,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2050059+560817 20260408.3362 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213639.84+560952.5,2461138.8362,12.83,0.05,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
ASASSN-V J213639.84+560952.5 20260408.3362 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 J212300.42+511244.0,2461138.8362,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212300.42+511244.0 20260408.3362 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211204.09+504444.3,2461138.8362,12.83,0.05,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
ASASSN-V J211204.09+504444.3 20260408.3362 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
NSVS 3407291,2461138.8362,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3407291 20260408.3362 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.1958+53.7317,2461138.8362,13.33,0.05,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
ATO J322.1958+53.7317 20260408.3362 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
NSVS J2050251+514807,2461138.8362,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2050251+514807 20260408.3362 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1728 Cyg,2461138.8362,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1728 Cyg 20260408.3362 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0560 Cep,2461138.8362,11.26,0.05,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
V0560 Cep 20260408.3362 11.26CV 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
ZTF J213557.53+535254.5,2461138.8362,13.16,0.05,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 J213557.53+535254.5 20260408.3362 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
NSVS J2104423+565659,2461138.8362,12.20,0.05,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
NSVS J2104423+565659 20260408.3362 12.20CV 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
ASASSN-V J204852.57+575127.2,2461138.8362,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204852.57+575127.2 20260408.3362 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204907.41+512204.0,2461138.8362,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204907.41+512204.0 20260408.3362 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213143.86+515313.0,2461138.8362,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213143.86+515313.0 20260408.3362 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214132.40+555039.4,2461138.8362,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214132.40+555039.4 20260408.3362 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212523.97+502118.5,2461138.8362,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212523.97+502118.5 20260408.3362 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
ATO J319.5768+53.5757,2461138.8362,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.5768+53.5757 20260408.3362 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 3409521,2461138.8362,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3409521 20260408.3362 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210659.79+511156.9,2461138.8362,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210659.79+511156.9 20260408.3362 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213712.13+530313.3,2461138.8362,12.83,0.05,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
ASASSN-V J213712.13+530313.3 20260408.3362 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
NSVS J2044576+575821,2461138.8362,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2044576+575821 20260408.3362 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212203.42+525208.9,2461138.8362,13.26,0.05,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 J212203.42+525208.9 20260408.3362 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
ZTF J213235.79+554457.1,2461138.8362,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213235.79+554457.1 20260408.3362 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2130209+502321,2461138.8362,12.04,0.05,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 J2130209+502321 20260408.3362 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
ZTF J213910.71+520757.6,2461138.8362,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213910.71+520757.6 20260408.3362 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BD+54 2511,2461138.8362,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BD+54 2511 20260408.3362 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2105270+570719,2461138.8362,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2105270+570719 20260408.3362 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V3137 Cyg,2461138.8362,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3137 Cyg 20260408.3362 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5844143,2461138.8362,12.78,0.05,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
NSVS 5844143 20260408.3362 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
NSVS 5974305,2461138.8362,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5974305 20260408.3362 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IRC +50368,2461138.8362,8.74,0.05,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
IRC +50368 20260408.3362 8.74CV 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
V2071 Cyg,2461138.8362,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2071 Cyg 20260408.3362 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J212653.64+531247.5,2461138.8362,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212653.64+531247.5 20260408.3362 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213730.20+505945.4,2461138.8362,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213730.20+505945.4 20260408.3362 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213627.25+495924.2,2461138.8362,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213627.25+495924.2 20260408.3362 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.2920+52.6435,2461138.8362,13.16,0.05,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
ATO J318.2920+52.6435 20260408.3362 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
ASASSN-V J213928.15+525718.5,2461138.8362,11.88,0.05,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
ASASSN-V J213928.15+525718.5 20260408.3362 11.88CV 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
ATO J318.5813+53.5672,2461138.8362,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.5813+53.5672 20260408.3362 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.3181+53.3201,2461138.8362,13.07,0.05,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
ATO J324.3181+53.3201 20260408.3362 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
ASASSN-V J210225.72+524729.9,2461138.8362,12.02,0.05,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
ASASSN-V J210225.72+524729.9 20260408.3362 12.02CV 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
ZTF J211813.98+532251.5,2461138.8362,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J211813.98+532251.5 20260408.3362 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5973713,2461138.8362,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5973713 20260408.3362 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461138.83655223 08.04.2026 08:04:28.113 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22723
Objects passed selection criteria: 22584
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 15622.2
Average stars matched: 13965.8 (89.3965 %)
Memory usage VmPeak: 124400 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 03:06:44 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: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461138.83655223 08.04.2026 08:04:28.113 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 350
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 50 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): 152266
Objects passed selection criteria: 151800
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 106240
Average stars matched: 95221 (89.6286 %)
Memory usage VmPeak: 1968688 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 03:09:13 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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: 2461138.83589852
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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:36.339 +54:00:29.17
Angular distance between the image centers 0.0099 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:39.098 +53:59:54.41
Angular distance between the image centers 0.0065 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 21:10:36.339 +54:00:29.17
Second-epoch second image center 21:10:39.098 +53:59:54.41
Angular distance between the image centers 0.01179 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.rb7WW2MUm0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.I0YJf7Fm5O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits &> /tmp/tmp.Vayju0uVGw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits &> /tmp/tmp.eTEVJWhP7g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat' -> 'wcsmag.cat'
Read 25856 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 303.1416 to 333.1026 deg, Dec +47.6313 to +59.3876 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 303.1416 to 333.1026 deg, Dec 47.6313 to 59.3876 deg
Loaded 21794 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): 12203 out of 13689 total matches.
Matched with Tycho-2 13689 out of 25856 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.933084
a=0.000000 b=1.000000 c=22.933084
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.4 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
3.3 pix fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
3.3 pix fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
14.2 mag. fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
14.2 mag. fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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.rb7WW2MUm0 (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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3218, passed=25856
Got 25856 stars (including 22610 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 25856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 972 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: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 25271 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 25269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 25269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.I0YJf7Fm5O (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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3203, passed=25854
Got 25854 stars (including 22628 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 25854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 974 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: 973 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.Vayju0uVGw (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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1239, passed=15103
Got 15103 stars (including 13850 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 15103 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 14646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
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 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 14645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 14645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 965 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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.eTEVJWhP7g (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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1193, passed=15064
Got 15064 stars (including 13860 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 15064 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 963 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: 962 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 14633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
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 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 14632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 14632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out10526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10558.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 33575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:35:54.93 +54:49:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34566_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 34566_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:44:45.07 +53:16:23.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35203_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 35203_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:44.88 +51:07:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05209_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 05209_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:36.26 +56:21:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16901_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 16901_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:43.86 +51:13:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09063_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 09063_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:50.36 +54:19:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09133_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 09133_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:55.92 +54:29:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14271_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 14271_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:23:29.54 +52:31:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19049_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 19049_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:26.81 +50:48:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06347_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 06347_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:09.38 +55:35:14.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23199_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 23199_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:33.49 +50:03:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23987_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 23987_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:06.59 +50:08:00.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10558_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 10558_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14743_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 14743_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:16.56 +52:08:54.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10526_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 10526_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 07575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:02.96 +54:55:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06115_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 06115_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:17:35.13 +55:59:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20179_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 20179_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:12:59.72 +50:37:36.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:16:28.12 +54:03:31.0
21:15:49.91 +54:01:34.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:36.339 +54:00:29.17
Angular distance between the image centers 0.0099 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:39.098 +53:59:54.41
Angular distance between the image centers 0.0065 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 21:10:36.339 +54:00:29.17
Second-epoch second image center 21:10:39.098 +53:59:54.41
Angular distance between the image centers 0.01179 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.PaxWrY6ZXG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.RLrrGsOD3d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits &> /tmp/tmp.IX1H6G4NEw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits &> /tmp/tmp.TXQSpxzBhx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat' -> 'wcsmag.cat'
Read 180620 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 303.1159 to 333.1394 deg, Dec +47.6313 to +59.3897 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 303.1159 to 333.1394 deg, Dec 47.6313 to 59.3897 deg
Loaded 21877 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): 9491 out of 14463 total matches.
Matched with Tycho-2 14463 out of 180620 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756732
a=0.000000 b=1.000000 c=22.756732
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 280 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
3.0 pix fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
3.0 pix fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Limiting magnitude estimates:
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
14.3 mag. fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
14.3 mag. fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (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.PaxWrY6ZXG (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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=28755, passed=180569
Got 180569 stars (including 151468 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 180569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 176761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 176760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 176759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.RLrrGsOD3d (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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=29011, passed=181061
Got 181061 stars (including 151708 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 181061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 678 to 748 (Dec 45.8 to 59.4)
Done reading UCAC5 zone files...
Matched 975 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: 973 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 177224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 678 to 748 (Dec 45.8 to 59.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 177222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 177222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.IX1H6G4NEw (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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=10804, passed=87363
Got 87363 stars (including 76469 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 87363 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 85171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
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 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 85171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 85171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 968 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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.TXQSpxzBhx (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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=10773, passed=87144
Got 87144 stars (including 76299 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 87144 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 964 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: 964 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 84569 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 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 84569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 84568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cyg-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-03-31_20.00sec_-5.00C_LIGHT_0157.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.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-02-Q2b1x1_030505_TTUQ2b1x1_26159_WjWX4xgk/wcs_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out136576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out227417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out227504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out227592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out229929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out218614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out225389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96902.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 44s
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: 38s
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Considering the candidate 204533_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204533_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:10:40.53 +55:35:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204535_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204535_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:28.26 +55:50:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 5.845 2188982931987007104 315.11779509910 +55.83756792499 13.6987 12.4635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204542_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204542_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:33:30.73 +50:18:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.080 2171330543377985024 323.37803009413 +50.31402232381 13.3401 12.8235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204545_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204545_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:22.80 +56:03:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204553_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204553_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:47:22.68 +56:31:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204561_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204561_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:00.25 +50:56:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204566_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204566_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:42:00.27 +54:59:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204567_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204567_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:53.69 +50:21:19.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 204568_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204568_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:22.72 +54:34:13.0 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 204569_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204569_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:04:41.38 +53:27:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.642 2176453309790528512 316.17152074832 +53.45342043173 12.9017 11.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204575_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:42.23 +53:11:15.1 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 204578_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204578_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:45.68 +52:02:20.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 204579_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204579_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:39:32.29 +55:48:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204581_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204581_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 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 204583_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204583_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 204587_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 204587_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:03.62 +57:05:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.607 2178923122149941248 319.76536779045 +57.09410092852 11.5682 9.9682 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 209148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:48.83 +57:05:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209495_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 209495_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:42:26.06 +57:45:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209526_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 209526_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:29:02.74 +51:14:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209569_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 209569_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:03:43.95 +53:15:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209825_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 209825_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:50.77 +57:27:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210393_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 210393_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:39:11.93 +57:29:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210466_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 210466_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:54:07.19 +57:09:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211066_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 211066_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:54.40 +53:19:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211733_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 211733_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:50:56.48 +56:56:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212589_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 212589_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:59.71 +49:57:25.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212779_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 212779_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:50:06.66 +56:48:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213304_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 213304_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:13:23.63 +58:02:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214449_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 214449_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:40.04 +57:45:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214714_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 214714_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:02:22.01 +56:39:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 214848_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 214848_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:13:50.23 +52:43:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215442_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 215442_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:11:30.22 +53:44:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215453_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 215453_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:43:00.51 +54:32:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215535_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 215535_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:34.87 +53:02:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215944_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 215944_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:43:57.50 +56:02:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216149_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 216149_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:46:17.79 +53:01:14.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 216193_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 216193_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:09.83 +51:04:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216422_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 216422_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:29:02.25 +55:26:11.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 216444_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 216444_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:11:19.00 +57:37:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217415_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 217415_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:56.10 +50:04:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217835_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 217835_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:49:35.01 +50:45:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218033_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218033_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:48.95 +51:48:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218272_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218272_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:30:40.42 +57:12:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218369_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218369_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:50:52.30 +55:02:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218506_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218506_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:13.78 +56:31:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218612_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218612_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:50:10.18 +56:47:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218614_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 218614_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 218667_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218667_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:43:22.92 +51:50:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218861_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 218861_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:59:13.24 +57:18:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219287_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219287_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:58.26 +49:57:10.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219325_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219325_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:55:02.39 +51:29:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.864 2169850811187888896 313.75986345690 +51.49787860954 13.1306 12.1407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219530_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219530_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:44.84 +52:28:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219774_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219774_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:07.33 +55:34:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219789_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219789_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:33:27.65 +56:16:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 219985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:58:24.15 +55:39:55.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220035_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 220035_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:31:07.32 +51:27:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220080_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 220080_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:39:32.81 +55:21:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220137_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 220137_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:03:54.98 +55:27:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220393_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 220393_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:29:42.21 +57:48:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220573_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 220573_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:04:04.24 +50:06:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221401_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 221401_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:10:04.94 +53:33:02.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221647_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 221647_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:48.58 +57:30:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 221805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:46:16.57 +53:19:16.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221962_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 221962_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:13.41 +51:53:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222064_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222064_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:28:43.49 +55:24:42.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:42:45.35 +54:05:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222269_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222269_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:44:23.17 +51:25:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222448_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222448_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:54:44.92 +57:39:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222452_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222452_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:11:20.58 +54:26:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222609_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222609_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:48:35.06 +51:54:17.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222616_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222616_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:44.86 +51:16:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222769_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 222769_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:36:51.49 +52:56:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223056_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 223056_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:43:06.88 +52:20:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223099_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 223099_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:31:18.73 +52:38:14.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223100_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 223100_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:33:30.03 +56:56:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223230_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 223230_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:48:08.92 +55:51:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224056_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224056_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:04:22.47 +56:30:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224075_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224075_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:32.72 +50:10:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224138_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224138_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:31.41 +57:38:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224147_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224147_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:57:43.69 +49:42:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224477_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224477_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:48:10.26 +55:50:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224862_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 224862_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:16:42.12 +51:00:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225354_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 225354_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:29:59.28 +52:57:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225389_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 225389_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225400_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 225400_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:47:35.80 +55:35:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225750_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 225750_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:25.60 +58:06:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225776_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 225776_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:58:13.59 +49:38:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226231_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226231_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:05:27.41 +54:03:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226357_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226357_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:47:46.35 +53:19:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226476_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226476_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:34.69 +51:29:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226549_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226549_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:33.41 +55:10:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226554_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226554_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:52:26.76 +54:39:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226924_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226924_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:41.64 +58:05:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226947_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226947_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:59:40.18 +55:32:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226955_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 226955_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:46:11.67 +54:23:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227120_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227120_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:25:52.68 +49:57:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227417_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227417_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:35.75 +55:06:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.420 2188807491162165504 315.14686894466 +55.10791939384 13.6470 12.8644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 227504_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227504_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:52:11.59 +50:58:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.114 2169740134172040960 313.04862175960 +50.97201257812 12.5043 10.9849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 227519_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227519_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:36:39.92 +56:19:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227592_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227592_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:28.26 +54:32:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 5.435 2188753271494474880 315.11527066348 +54.54195913191 13.8844 13.2157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 227663_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227663_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:22:23.43 +55:35:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227825_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 227825_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:57:10.66 +54:28:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228146_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 228146_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:51:47.76 +52:27:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228337_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 228337_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:53:16.18 +58:02:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228560_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 228560_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:21:37.04 +49:47:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228849_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 228849_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:22.47 +55:33:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229064_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 229064_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:28:59.01 +54:41:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229722_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 229722_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:43:48.06 +56:03:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229850_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 229850_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:35:41.83 +53:21:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229888_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 229888_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:50:40.68 +57:10:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229929_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 229929_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:50.01 +53:32:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.285 2172937342187078272 321.70914689160 +53.54041093847 11.9965 10.3192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 230366_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 230366_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:32.80 +55:06:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230386_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 230386_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:25:55.96 +56:36:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230503_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 230503_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:04:31.70 +50:15:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230581_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 230581_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:01.43 +53:47:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230774_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 230774_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:41:00.71 +54:42:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231198_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231198_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:47:49.28 +55:26:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231202_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231202_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:29.54 +56:19:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 4.755 2178078692917957760 324.62398095868 +56.32411245258 12.7800 11.2529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 231355_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231355_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:50.82 +57:49:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231362_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231362_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:07:46.68 +55:30:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231423_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231423_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:53:47.20 +56:25:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231546_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231546_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:09:16.49 +52:16:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.364 2169534117475203584 317.31783970921 +52.27546895130 12.8155 11.2942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 231700_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231700_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:08:59.15 +56:13:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.933 2189323265196189312 317.24572635901 +56.22654165710 12.2261 10.4659 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 231718_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231718_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:30:35.09 +54:36:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231810_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 231810_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:56:07.65 +56:41:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112291_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 112291_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 198831_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 198831_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:25.07 +57:37:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.320 2179185424394032256 323.10524886325 +57.62048390361 12.8652 11.4494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192388_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 192388_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:16.85 +52:28:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.602 2175392246710859776 319.82085294099 +52.46820940441 10.9361 9.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192500_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 192500_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:21.85 +49:57:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129787_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 129787_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 111684_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 111684_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 195069_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 195069_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:36:56.96 +50:20:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171687_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 171687_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 134154_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 134154_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 79640_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 79640_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:05:22.35 +54:03:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121360_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 121360_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 172036_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 172036_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 127589_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 127589_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:08:25.36 +51:23:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135032_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 135032_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:23.76 +50:03:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14224_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 14224_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 143509_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 143509_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 46334_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 46334_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:09.37 +55:35:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131514_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 131514_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 105747_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 105747_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:07.63 +52:01:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142145_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 142145_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:17:17.52 +50:45:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22744_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 22744_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:54.17 +57:22:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93239_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 93239_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:46.07 +53:06:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60665_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 60665_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:22.05 +54:51:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171963_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 171963_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 110292_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 110292_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 37466_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 37466_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 132898_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 132898_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 149254_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 149254_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:15:30.60 +51:07:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84016_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 84016_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 13460_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 13460_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 89358_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 89358_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:22:16.01 +53:19:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 141805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:33:56.77 +50:24:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82591_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 82591_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 191316_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 191316_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:40:32.90 +51:38:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149319_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 149319_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 56238_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 56238_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:02.85 +54:55:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118736_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 118736_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 55363_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 55363_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 111297_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 111297_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 17889_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 17889_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:42:25.68 +57:22:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51830_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 51830_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:17:07.56 +55:30:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129635_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 129635_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 75957_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 75957_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 95780_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 95780_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 27382_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 27382_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 109237_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 109237_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65541_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 65541_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:23:53.38 +54:35:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177359_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 177359_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 64886_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 64886_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 109080_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 109080_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117091_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 117091_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 103722_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 103722_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:23:29.54 +52:31:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57771_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 57771_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:53.30 +55:08:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87887_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 87887_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141563_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 141563_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173364_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 173364_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179766_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 179766_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66177_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 66177_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51746_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 51746_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 149189_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 149189_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 80771_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 80771_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44951_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 44951_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36288_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 36288_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127175_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 127175_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141110_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 141110_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 21978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 105683_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 105683_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:29:18.41 +52:13:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67156_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 67156_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:34.72 +54:09:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78737_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 78737_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 61368_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 61368_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:48.32 +54:40:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 121978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 22006_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 22006_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:23:38.48 +57:27:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.329 2178948617076691072 320.91048443733 +57.46086571505 12.7767 11.3829 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121939_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 121939_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 196157_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 196157_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:42:16.83 +52:03:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.736 2182275563162137216 310.56907608568 +52.05042984724 12.2494 10.7866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 43968_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 43968_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 73100_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 73100_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 78617_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 78617_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:16:28.12 +54:03:30.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 118280_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 118280_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:27.64 +51:22:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23867_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 23867_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:24:40.24 +57:18:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32676_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 32676_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 24584_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 24584_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:42:03.38 +56:54:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145157_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 145157_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:21:20.92 +50:50:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20224_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 20224_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 106674_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 106674_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:28:03.55 +52:13:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130176_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 130176_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 110805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 110805_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 63123_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 63123_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:08:38.66 +54:55:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45086_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 45086_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:17:35.11 +55:59:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120757_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 120757_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:43.85 +51:13:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38846_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 38846_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 57750_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 57750_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:35:54.85 +54:49:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147113_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 147113_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:44.89 +51:07:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44349_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 44349_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:41:03.79 +55:30:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69572_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 69572_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:50.38 +54:19:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106095_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 106095_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:34:16.52 +52:08:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137375_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 137375_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 179292_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 179292_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:19.19 +49:50:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 38978_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:36.26 +56:21:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143451_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 143451_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:19:26.81 +50:48:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134613_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 134613_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:13:05.35 +50:25:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85172_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 85172_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 40263_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 40263_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 148315_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 148315_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87553_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 87553_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 91365_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 91365_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:07:19.11 +53:24:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18776_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 18776_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 96902_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 96902_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 62044_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 62044_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:31:09.46 +54:38:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43757_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 43757_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 139564_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 139564_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103402_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 103402_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 29275_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 29275_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:33:29.63 +56:46:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57850_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 57850_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 17442_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 17442_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:22:36.40 +57:49:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 30148_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 93759_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 93759_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:42:10.69 +53:19:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173161_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 173161_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:00:33.50 +50:03:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93211_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 93211_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 78940_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 78940_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:38:53.07 +53:29:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170967_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 170967_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113417_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 113417_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 138068_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 138068_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:47.73 +50:21:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171300_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 171300_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 79891_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 79891_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:15:49.91 +54:01:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 177071_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 177071_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 63389_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 63389_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:37:40.54 +54:24:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193712_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 193712_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:56.48 +50:19:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.382 2171890572758073472 320.23553397529 +50.32458265052 12.3211 10.7249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 136576_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 136576_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:16:25.27 +50:29:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.352 2166138168435482368 319.10516034290 +50.48525490179 12.1915 10.4565 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193682_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 193682_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:54:26.59 +50:29:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.290 2169665371681283584 313.60991533241 +50.48355477967 11.4930 9.8729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52602_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 52602_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:14:33.21 +55:30:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89057_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 89057_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 199490_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 199490_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:35:15.60 +53:57:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125195_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 125195_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 66836_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 66836_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:26:55.93 +54:29:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121851_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 121851_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:39:18.83 +51:07:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141947_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 141947_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:20:17.69 +50:41:09.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 134985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 134985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 174556_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 174556_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:01:06.60 +50:08:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62367_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 62367_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:36:34.54 +54:30:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103144_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 103144_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
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Considering the candidate 65727_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 65727_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:39:46.42 +54:12:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192629_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 192629_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:32:55.65 +51:18:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88687_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 88687_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94836_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 94836_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 20:44:45.13 +53:16:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39605_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 39605_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:15:14.19 +56:18:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86185_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 86185_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107436_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 107436_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:31:46.44 +52:04:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80512_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 80512_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:27:09.82 +53:39:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.496 2172938411643343232 321.79160074251 +53.66099225106 12.5523 11.0749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82588_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 82588_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138496_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 138496_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:12:59.72 +50:37:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 102985_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125047_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 125047_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:04:54.94 +51:34:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88765_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 88765_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177980_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
The candidate 177980_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158 did not pass the final checks
**** FOUND 21:18:28.78 +50:08:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114724_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
Preparing report for the candidate 114724_fd_Cyg-02-Q2b1x1_2026-04-08_03-04-28_20.00sec_-4.90C_LIGHT_0158
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 88s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:16:28.12 +54:03:31.0
21:15:49.91 +54:01:34.5
21:02:25.95 +52:47:29.7
21:13:07.37 +52:38:49.1
21:39:10.17 +52:07:56.8
21:22:09.38 +52:11:59.0
21:27:04.21 +52:04:27.0
21:27:48.24 +52:01:06.5
21:31:43.61 +51:53:12.6
21:32:33.92 +51:50:54.9
21:25:26.55 +51:58:18.4
21:26:33.26 +51:55:25.3
21:37:35.94 +51:41:07.0
21:37:00.26 +51:37:15.6
21:35:05.90 +51:28:34.2
21:31:53.69 +51:29:47.7
21:36:18.76 +51:13:46.4
21:35:52.00 +51:14:42.7
20:50:25.66 +51:48:08.6
21:37:29.83 +50:59:48.2
21:23:00.47 +51:12:44.0
21:00:10.65 +51:21:55.1
21:28:47.99 +50:58:38.7
20:49:07.71 +51:22:05.3
20:52:44.50 +49:52:08.3
21:17:21.03 +49:59:35.8
21:26:14.71 +50:07:06.4
21:37:46.76 +57:44:09.5
21:36:26.67 +49:59:27.9
21:25:23.60 +50:21:18.9
21:30:20.51 +50:23:24.7
21:12:04.09 +50:44:45.0
21:27:00.33 +50:32:33.1
21:35:40.68 +57:48:37.4
21:31:24.29 +50:32:50.6
21:06:59.72 +51:11:56.2
21:31:02.68 +50:49:55.9
21:33:14.83 +50:47:40.5
21:05:41.46 +49:52:06.2
21:16:57.69 +49:58:40.2
21:17:55.91 +49:45:25.0
21:18:11.72 +49:46:51.5
21:05:48.14 +49:57:34.1
21:23:18.25 +49:47:26.4
21:30:36.42 +49:51:19.4
21:34:50.85 +49:46:19.1
21:24:01.75 +50:11:07.0
20:44:58.20 +57:58:18.0
20:48:52.84 +57:51:23.1
21:32:46.76 +54:17:26.4
21:36:47.16 +57:12:30.3
20:59:38.43 +55:57:12.1
21:16:41.75 +57:10:39.6
21:05:27.00 +57:07:16.3
21:04:42.24 +56:56:56.0
21:36:39.59 +56:09:50.3
21:13:49.96 +56:30:32.8
21:41:31.70 +55:50:37.2
21:41:27.16 +55:47:25.7
21:32:35.30 +55:44:54.8
21:36:10.08 +55:41:09.0
20:50:05.99 +56:08:17.1
20:59:07.99 +55:42:36.3
21:25:23.23 +55:09:00.0
21:18:18.31 +55:15:34.8
21:22:41.53 +54:38:12.1
21:34:28.14 +54:19:36.9
21:35:57.23 +53:52:51.5
21:09:43.66 +54:10:28.5
21:28:46.77 +53:43:51.4
21:23:25.08 +53:43:57.1
21:37:16.15 +53:19:07.1
21:25:31.04 +53:36:12.1
21:40:26.91 +53:10:31.4
21:18:22.01 +53:34:20.8
21:14:19.68 +53:34:00.1
21:37:11.74 +53:03:09.4
21:14:14.27 +53:30:57.0
21:39:27.76 +52:57:16.7
21:18:14.35 +53:22:48.6
21:26:53.54 +53:12:45.5
21:22:02.36 +53:04:20.4
20:52:26.89 +53:12:04.3
21:22:03.31 +52:52:07.7
########### Completed Cyg-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:15:49.91 +54:01:34.5
21:16:28.12 +54:03:31.0
21:32:46.76 +54:17:26.4
20:59:38.43 +55:57:12.1
21:26:33.26 +51:55:25.3
21:28:47.99 +50:58:38.7
21:25:26.55 +51:58:18.4
21:17:55.91 +49:45:25.0
21:26:14.71 +50:07:06.4
21:36:18.76 +51:13:46.4
21:05:48.14 +49:57:34.1
21:35:40.68 +57:48:37.4
21:31:24.29 +50:32:50.6
20:52:44.50 +49:52:08.3
21:18:11.72 +49:46:51.5
21:27:48.24 +52:01:06.5
21:13:49.96 +56:30:32.8
21:17:21.03 +49:59:35.8
21:40:26.91 +53:10:31.4
21:37:46.76 +57:44:09.5
21:25:31.04 +53:36:12.1
21:33:14.83 +50:47:40.5
21:31:53.69 +51:29:47.7
21:25:23.23 +55:09:00.0
21:32:33.92 +51:50:54.9
21:00:10.65 +51:21:55.1
21:09:43.66 +54:10:28.5
20:52:26.89 +53:12:04.3
21:16:41.75 +57:10:39.6
21:27:04.21 +52:04:27.0
21:34:50.85 +49:46:19.1
21:22:41.53 +54:38:12.1
21:22:09.38 +52:11:59.0
21:35:05.90 +51:28:34.2
21:14:14.27 +53:30:57.0
21:27:00.33 +50:32:33.1
21:23:18.25 +49:47:26.4
21:24:01.75 +50:11:07.0
21:34:28.14 +54:19:36.9
20:59:07.99 +55:42:36.3
21:31:02.68 +50:49:55.9
21:23:25.08 +53:43:57.1
20:50:05.99 +56:08:17.1
21:36:39.59 +56:09:50.3
21:23:00.47 +51:12:44.0
21:12:04.09 +50:44:45.0
21:36:47.16 +57:12:30.3
21:28:46.77 +53:43:51.4
20:50:25.66 +51:48:08.6
21:35:52.00 +51:14:42.7
21:36:10.08 +55:41:09.0
21:35:57.23 +53:52:51.5
21:04:42.24 +56:56:56.0
20:48:52.84 +57:51:23.1
20:49:07.71 +51:22:05.3
21:31:43.61 +51:53:12.6
21:41:31.70 +55:50:37.2
21:25:23.60 +50:21:18.9
21:18:22.01 +53:34:20.8
21:41:27.16 +55:47:25.7
21:06:59.72 +51:11:56.2
21:37:11.74 +53:03:09.4
20:44:58.20 +57:58:18.0
21:22:03.31 +52:52:07.7
21:32:35.30 +55:44:54.8
21:30:20.51 +50:23:24.7
21:39:10.17 +52:07:56.8
21:18:18.31 +55:15:34.8
21:05:27.00 +57:07:16.3
21:22:02.36 +53:04:20.4
21:05:41.46 +49:52:06.2
21:37:35.94 +51:41:07.0
21:16:57.69 +49:58:40.2
21:30:36.42 +49:51:19.4
21:26:53.54 +53:12:45.5
21:37:29.83 +50:59:48.2
21:36:26.67 +49:59:27.9
21:13:07.37 +52:38:49.1
21:39:27.76 +52:57:16.7
21:14:19.68 +53:34:00.1
21:37:16.15 +53:19:07.1
21:02:25.95 +52:47:29.7
21:18:14.35 +53:22:48.6
21:37:00.26 +51:37:15.6
###################################################################################
21:15:49.91 +54:01:34.5 -- not an asteroid (will add it to exclusion list)
21:16:28.12 +54:03:31.0 -- not an asteroid (will add it to exclusion list)
21:32:46.76 +54:17:26.4 -- not an asteroid (will add it to exclusion list)
20:59:38.43 +55:57:12.1 -- not an asteroid (will add it to exclusion list)
21:26:33.26 +51:55:25.3 -- not an asteroid (will add it to exclusion list)
21:28:47.99 +50:58:38.7 -- not an asteroid (will add it to exclusion list)
21:25:26.55 +51:58:18.4 -- not an asteroid (will add it to exclusion list)
21:17:55.91 +49:45:25.0 -- not an asteroid (will add it to exclusion list)
21:26:14.71 +50:07:06.4 -- not an asteroid (will add it to exclusion list)
21:36:18.76 +51:13:46.4 -- not an asteroid (will add it to exclusion list)
21:05:48.14 +49:57:34.1 -- not an asteroid (will add it to exclusion list)
21:35:40.68 +57:48:37.4 -- not an asteroid (will add it to exclusion list)
21:31:24.29 +50:32:50.6 -- not an asteroid (will add it to exclusion list)
20:52:44.50 +49:52:08.3 -- not an asteroid (will add it to exclusion list)
21:18:11.72 +49:46:51.5 -- not an asteroid (will add it to exclusion list)
21:27:48.24 +52:01:06.5 -- not an asteroid (will add it to exclusion list)
21:13:49.96 +56:30:32.8 -- not an asteroid (will add it to exclusion list)
21:17:21.03 +49:59:35.8 -- not an asteroid (will add it to exclusion list)
21:40:26.91 +53:10:31.4 -- not an asteroid (will add it to exclusion list)
21:37:46.76 +57:44:09.5 -- not an asteroid (will add it to exclusion list)
21:25:31.04 +53:36:12.1 -- not an asteroid (will add it to exclusion list)
21:33:14.83 +50:47:40.5 -- not an asteroid (will add it to exclusion list)
21:31:53.69 +51:29:47.7 -- not an asteroid (will add it to exclusion list)
21:25:23.23 +55:09:00.0 -- not an asteroid (will add it to exclusion list)
21:32:33.92 +51:50:54.9 -- not an asteroid (will add it to exclusion list)
21:00:10.65 +51:21:55.1 -- not an asteroid (will add it to exclusion list)
21:09:43.66 +54:10:28.5 -- not an asteroid (will add it to exclusion list)
20:52:26.89 +53:12:04.3 -- not an asteroid (will add it to exclusion list)
21:16:41.75 +57:10:39.6 -- not an asteroid (will add it to exclusion list)
21:27:04.21 +52:04:27.0 -- not an asteroid (will add it to exclusion list)
21:34:50.85 +49:46:19.1 -- not an asteroid (will add it to exclusion list)
21:22:41.53 +54:38:12.1 -- not an asteroid (will add it to exclusion list)
21:22:09.38 +52:11:59.0 -- not an asteroid (will add it to exclusion list)
21:35:05.90 +51:28:34.2 -- not an asteroid (will add it to exclusion list)
21:14:14.27 +53:30:57.0 -- not an asteroid (will add it to exclusion list)
21:27:00.33 +50:32:33.1 -- not an asteroid (will add it to exclusion list)
21:23:18.25 +49:47:26.4 -- not an asteroid (will add it to exclusion list)
21:24:01.75 +50:11:07.0 -- not an asteroid (will add it to exclusion list)
21:34:28.14 +54:19:36.9 -- not an asteroid (will add it to exclusion list)
20:59:07.99 +55:42:36.3 -- not an asteroid (will add it to exclusion list)
21:31:02.68 +50:49:55.9 -- not an asteroid (will add it to exclusion list)
21:23:25.08 +53:43:57.1 -- not an asteroid (will add it to exclusion list)
20:50:05.99 +56:08:17.1 -- not an asteroid (will add it to exclusion list)
21:36:39.59 +56:09:50.3 -- not an asteroid (will add it to exclusion list)
21:23:00.47 +51:12:44.0 -- not an asteroid (will add it to exclusion list)
21:12:04.09 +50:44:45.0 -- not an asteroid (will add it to exclusion list)
21:36:47.16 +57:12:30.3 -- not an asteroid (will add it to exclusion list)
21:28:46.77 +53:43:51.4 -- not an asteroid (will add it to exclusion list)
20:50:25.66 +51:48:08.6 -- not an asteroid (will add it to exclusion list)
21:35:52.00 +51:14:42.7 -- not an asteroid (will add it to exclusion list)
21:36:10.08 +55:41:09.0 -- not an asteroid (will add it to exclusion list)
21:35:57.23 +53:52:51.5 -- not an asteroid (will add it to exclusion list)
21:04:42.24 +56:56:56.0 -- not an asteroid (will add it to exclusion list)
20:48:52.84 +57:51:23.1 -- not an asteroid (will add it to exclusion list)
20:49:07.71 +51:22:05.3 -- not an asteroid (will add it to exclusion list)
21:31:43.61 +51:53:12.6 -- not an asteroid (will add it to exclusion list)
21:41:31.70 +55:50:37.2 -- not an asteroid (will add it to exclusion list)
21:25:23.60 +50:21:18.9 -- not an asteroid (will add it to exclusion list)
21:18:22.01 +53:34:20.8 -- not an asteroid (will add it to exclusion list)
21:41:27.16 +55:47:25.7 -- not an asteroid (will add it to exclusion list)
21:06:59.72 +51:11:56.2 -- not an asteroid (will add it to exclusion list)
21:37:11.74 +53:03:09.4 -- not an asteroid (will add it to exclusion list)
20:44:58.20 +57:58:18.0 -- not an asteroid (will add it to exclusion list)
21:22:03.31 +52:52:07.7 -- not an asteroid (will add it to exclusion list)
21:32:35.30 +55:44:54.8 -- not an asteroid (will add it to exclusion list)
21:30:20.51 +50:23:24.7 -- not an asteroid (will add it to exclusion list)
21:39:10.17 +52:07:56.8 -- not an asteroid (will add it to exclusion list)
21:18:18.31 +55:15:34.8 -- not an asteroid (will add it to exclusion list)
21:05:27.00 +57:07:16.3 -- not an asteroid (will add it to exclusion list)
21:22:02.36 +53:04:20.4 -- not an asteroid (will add it to exclusion list)
21:05:41.46 +49:52:06.2 -- not an asteroid (will add it to exclusion list)
21:37:35.94 +51:41:07.0 -- not an asteroid (will add it to exclusion list)
21:16:57.69 +49:58:40.2 -- not an asteroid (will add it to exclusion list)
21:30:36.42 +49:51:19.4 -- not an asteroid (will add it to exclusion list)
21:26:53.54 +53:12:45.5 -- not an asteroid (will add it to exclusion list)
21:37:29.83 +50:59:48.2 -- not an asteroid (will add it to exclusion list)
21:36:26.67 +49:59:27.9 -- not an asteroid (will add it to exclusion list)
21:13:07.37 +52:38:49.1 -- not an asteroid (will add it to exclusion list)
21:39:27.76 +52:57:16.7 -- not an asteroid (will add it to exclusion list)
21:14:19.68 +53:34:00.1 -- not an asteroid (will add it to exclusion list)
21:37:16.15 +53:19:07.1 -- not an asteroid (will add it to exclusion list)
21:02:25.95 +52:47:29.7 -- not an asteroid (will add it to exclusion list)
21:18:14.35 +53:22:48.6 -- not an asteroid (will add it to exclusion list)
21:37:00.26 +51:37:15.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:44:58.20 +57:58:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:52.84 +57:51:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:07.71 +51:22:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:05.99 +56:08:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:25.66 +51:48:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:26.89 +53:12:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:44.50 +49:52:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:07.99 +55:42:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:38.43 +55:57:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:10.65 +51:21:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:25.95 +52:47:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:42.24 +56:56:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:27.00 +57:07:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:41.46 +49:52:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:48.14 +49:57:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:59.72 +51:11:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:43.66 +54:10:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:04.09 +50:44:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:07.37 +52:38:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:49.96 +56:30:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:14.27 +53:30:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:19.68 +53:34:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:49.91 +54:01:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:28.12 +54:03:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:41.75 +57:10:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:57.69 +49:58:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:21.03 +49:59:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:55.91 +49:45:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:11.72 +49:46:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:14.35 +53:22:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:18.31 +55:15:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:22.01 +53:34:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:02.36 +53:04:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:03.31 +52:52:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:09.38 +52:11:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:41.53 +54:38:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:00.47 +51:12:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:18.25 +49:47:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:25.08 +53:43:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:01.75 +50:11:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:23.23 +55:09:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:23.60 +50:21:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:26.55 +51:58:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:31.04 +53:36:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:14.71 +50:07:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:33.26 +51:55:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.54 +53:12:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:00.33 +50:32:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:04.21 +52:04:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:48.24 +52:01:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:46.77 +53:43:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:47.99 +50:58:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:20.51 +50:23:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:36.42 +49:51:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:02.68 +50:49:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:24.29 +50:32:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:43.61 +51:53:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:53.69 +51:29:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:33.92 +51:50:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:35.30 +55:44:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:46.76 +54:17:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:14.83 +50:47:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:28.14 +54:19:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:50.85 +49:46:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:05.90 +51:28:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:40.68 +57:48:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:52.00 +51:14:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:57.23 +53:52:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:10.08 +55:41:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:18.76 +51:13:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:26.67 +49:59:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:39.59 +56:09:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:47.16 +57:12:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:00.26 +51:37:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:11.74 +53:03:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:16.15 +53:19:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:29.83 +50:59:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:35.94 +51:41:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.76 +57:44:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:10.17 +52:07:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:27.76 +52:57:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:26.91 +53:10:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:27.16 +55:47:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:31.70 +55:50:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:44:58.20 +57:58:18.0 -- a known variable star
20:48:52.84 +57:51:23.1 -- a known variable star
20:49:07.71 +51:22:05.3 -- a known variable star
20:50:05.99 +56:08:17.1 -- a known variable star
20:50:25.66 +51:48:08.6 -- a known variable star
20:52:26.89 +53:12:04.3 -- a known variable star
20:52:44.50 +49:52:08.3 -- a known variable star
20:59:07.99 +55:42:36.3 -- a known variable star
20:59:38.43 +55:57:12.1 -- not a known variable star
21:00:10.65 +51:21:55.1 -- a known variable star
21:02:25.95 +52:47:29.7 -- a known variable star
21:04:42.24 +56:56:56.0 -- a known variable star
21:05:27.00 +57:07:16.3 -- a known variable star
21:05:41.46 +49:52:06.2 -- a known variable star
21:05:48.14 +49:57:34.1 -- not a known variable star
21:06:59.72 +51:11:56.2 -- a known variable star
21:09:43.66 +54:10:28.5 -- a known variable star
21:12:04.09 +50:44:45.0 -- a known variable star
21:13:07.37 +52:38:49.1 -- not a known variable star
21:13:49.96 +56:30:32.8 -- a known variable star
21:14:14.27 +53:30:57.0 -- a known variable star
21:14:19.68 +53:34:00.1 -- not a known variable star
21:15:49.91 +54:01:34.5 -- a known variable star
21:16:28.12 +54:03:31.0 -- a known variable star
21:16:41.75 +57:10:39.6 -- a known variable star
21:16:57.69 +49:58:40.2 -- a known variable star
21:17:21.03 +49:59:35.8 -- a known variable star
21:17:55.91 +49:45:25.0 -- a known variable star
21:18:11.72 +49:46:51.5 -- not a known variable star
21:18:14.35 +53:22:48.6 -- a known variable star
21:18:18.31 +55:15:34.8 -- a known variable star
21:18:22.01 +53:34:20.8 -- not a known variable star
21:22:02.36 +53:04:20.4 -- a known variable star
21:22:03.31 +52:52:07.7 -- a known variable star
21:22:09.38 +52:11:59.0 -- a known variable star
21:22:41.53 +54:38:12.1 -- a known variable star
21:23:00.47 +51:12:44.0 -- a known variable star
21:23:18.25 +49:47:26.4 -- a known variable star
21:23:25.08 +53:43:57.1 -- a known variable star
21:24:01.75 +50:11:07.0 -- not a known variable star
21:25:23.23 +55:09:00.0 -- a known variable star
21:25:23.60 +50:21:18.9 -- a known variable star
21:25:26.55 +51:58:18.4 -- not a known variable star
21:25:31.04 +53:36:12.1 -- a known variable star
21:26:14.71 +50:07:06.4 -- a known variable star
21:26:33.26 +51:55:25.3 -- a known variable star
21:26:53.54 +53:12:45.5 -- a known variable star
21:27:00.33 +50:32:33.1 -- a known variable star
21:27:04.21 +52:04:27.0 -- not a known variable star
21:27:48.24 +52:01:06.5 -- a known variable star
21:28:46.77 +53:43:51.4 -- not a known variable star
21:28:47.99 +50:58:38.7 -- a known variable star
21:30:20.51 +50:23:24.7 -- a known variable star
21:30:36.42 +49:51:19.4 -- a known variable star
21:31:02.68 +50:49:55.9 -- not a known variable star
21:31:24.29 +50:32:50.6 -- a known variable star
21:31:43.61 +51:53:12.6 -- a known variable star
21:31:53.69 +51:29:47.7 -- a known variable star
21:32:33.92 +51:50:54.9 -- a known variable star
21:32:35.30 +55:44:54.8 -- a known variable star
21:32:46.76 +54:17:26.4 -- not a known variable star
21:33:14.83 +50:47:40.5 -- a known variable star
21:34:28.14 +54:19:36.9 -- not a known variable star
21:34:50.85 +49:46:19.1 -- a known variable star
21:35:05.90 +51:28:34.2 -- not a known variable star
21:35:40.68 +57:48:37.4 -- a known variable star
21:35:52.00 +51:14:42.7 -- a known variable star
21:35:57.23 +53:52:51.5 -- a known variable star
21:36:10.08 +55:41:09.0 -- a known variable star
21:36:18.76 +51:13:46.4 -- a known variable star
21:36:26.67 +49:59:27.9 -- a known variable star
21:36:39.59 +56:09:50.3 -- a known variable star
21:36:47.16 +57:12:30.3 -- a known variable star
21:37:00.26 +51:37:15.6 -- a known variable star
21:37:11.74 +53:03:09.4 -- a known variable star
21:37:16.15 +53:19:07.1 -- not a known variable star
21:37:29.83 +50:59:48.2 -- a known variable star
21:37:35.94 +51:41:07.0 -- a known variable star
21:37:46.76 +57:44:09.5 -- a known variable star
21:39:10.17 +52:07:56.8 -- a known variable star
21:39:27.76 +52:57:16.7 -- a known variable star
21:40:26.91 +53:10:31.4 -- a known variable star
21:41:27.16 +55:47:25.7 -- a known variable star
21:41:31.70 +55:50:37.2 -- a known variable star
Found 15 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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84 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 84 (excluding asteroids and hot pixels, 15 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)2461138.83589852 -observatory V36
23:29:44.23 -05:39:47.3 Mercury (0.3mag)
02:31:40.03 +14:46:42.5 Venus (-3.9mag)
23:56:01.79 -01:32:15.1 Mars (1.2mag)
07:09:28.07 +22:51:16.1 Jupiter (-2.2mag)
00:25:44.10 +00:27:22.2 Saturn (0.9mag)
03:46:08.24 +19:42:26.5 Uranus (5.8mag)
00:09:49.23 -00:21:49.4 Neptune (7.8mag)
20:33:21.89 -22:52:27.3 Pluto (14.5mag)
17:52:11.03 -28:54:32.0 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 03:06 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461138.83589852:
07:09:22.29 +22:51:25.4 Io (5.7mag)
07:09:19.48 +22:51:35.8 Europa (5.9mag)
07:09:48.48 +22:50:34.9 Ganymede (5.3mag)
07:08:53.34 +22:52:25.7 Callisto (6.5mag)
07:13:06.68 +22:42:39.1 Himalia (15.3mag)
07:09:29.61 +22:51:15.0 Thebe (16.2mag)
07:13:07.50 +23:11:51.6 Elara (17.3mag)
07:07:49.65 +23:35:17.0 Pasiphae (17.4mag)
07:17:57.42 +22:48:27.8 Carme (18.4mag)
00:25:47.45 +00:27:12.4 Titan (8.8mag)
00:25:49.53 +00:27:22.8 Rhea (10.1mag)
00:25:39.77 +00:28:40.1 Iapetus (11.5mag)
00:25:53.17 +00:27:07.6 Hyperion (14.8mag)
00:27:26.81 +00:36:58.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 03:06 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.83589852:
14:59:13.14 -10:16:07.7 JWST
14:38:06.84 +56:07:26.8 Chandra
08:27:27.12 -46:12:52.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 03:06 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.83589852 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:20.73 -28:20:56.3 13.9mag P/2010 H2 (Vales)
05:01:27.96 -70:02:16.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:56.07 +31:23:18.0 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.01 +09:37:47.7 17.6mag C/2021 G2 (ATLAS)
23:08:01.64 +28:56:29.5 17.0mag C/2022 E2 (ATLAS)
04:20:24.90 +25:49:31.5 15.9mag C/2022 N2 (PANSTARRS)
09:02:06.21 +31:56:26.7 16.2mag C/2022 QE78 (ATLAS)
08:30:08.78 -00:59:21.7 17.3mag C/2022 R6 (PANSTARRS)
18:55:16.12 +17:52:48.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:57.34 -11:37:53.0 17.6mag P/2023 B1 (PANSTARRS)
09:11:34.61 -13:08:26.2 17.6mag C/2023 F3 (ATLAS)
21:45:59.22 +62:28:51.3 17.5mag C/2023 H5 (Lemmon)
19:25:03.46 -03:37:46.1 14.2mag C/2023 R1 (PANSTARRS)
21:41:48.64 +84:52:58.0 17.8mag C/2023 X2 (Lemmon)
06:15:02.28 +63:33:47.9 17.1mag C/2024 A1 (ATLAS)
04:56:09.29 +15:28:19.4 10.5mag C/2024 E1 (Wierzchos)
16:23:55.17 +05:07:49.8 17.4mag C/2024 G6 (ATLAS)
20:18:21.25 +13:14:10.8 14.7mag C/2024 J3 (ATLAS)
03:19:36.48 -23:34:43.3 16.4mag C/2024 T5 (ATLAS)
05:10:23.57 +47:15:27.5 17.7mag C/2025 J1 (Borisov)
14:10:30.33 +39:28:16.8 14.9mag C/2025 L1 (ATLAS)
03:13:31.17 -25:03:24.4 17.8mag C/2025 Q3 (ATLAS)
22:59:52.16 +19:48:23.4 9.7mag C/2025 R3 (PANSTARRS)
12:57:27.39 +02:31:54.6 17.5mag C/2025 Y1 (ATLAS)
02:05:45.62 +03:57:19.7 9.7mag C/2026 A1 (MAPS)
23:37:16.57 +35:42:30.8 14.3mag C/2026 B2 (Sun-Gao)
18:27:59.09 -10:06:55.3 12.3mag 10P/Tempel
15:10:18.75 +03:56:10.0 13.3mag 24P/Schaumasse
11:05:03.59 -01:47:11.1 15.7mag 29P/Schwassmann-Wachmann
17:57:55.79 -09:54:22.5 17.8mag 40P/Vaisala
10:38:25.46 -04:45:01.3 16.8mag 43P/Wolf-Harrington
01:36:50.81 +16:10:10.1 17.2mag 47P/Ashbrook-Jackson
06:57:00.50 +38:38:07.1 17.0mag 63P/Wild
23:19:08.47 -12:23:13.8 15.7mag 65P/Gunn
03:43:09.01 +18:31:58.9 15.9mag 76P/West-Kohoutek-Ikemura
00:48:44.65 +06:42:45.3 14.4mag 78P/Gehrels
22:39:20.98 -11:38:51.4 14.5mag 88P/Howell
01:49:01.57 +18:33:01.5 15.1mag 93P/Lovas
04:40:43.05 +31:51:23.9 16.3mag 123P/West-Hartley
08:19:59.12 +41:54:00.3 16.2mag 124P/Mrkos
02:21:27.96 +13:30:13.0 16.4mag 128P/Shoemaker-Holt
02:32:33.78 +13:31:56.8 17.5mag 131P/Mueller
00:46:37.51 +10:26:28.4 11.1mag 141P/Machholz
00:56:26.10 +01:59:49.5 11.1mag 141P-A/Machholz
23:45:45.54 -01:44:47.3 13.8mag 141P-D/Machholz
01:25:53.38 +03:41:41.0 17.9mag 141P-I/Machholz
00:41:04.56 -05:21:28.8 15.2mag 162P/SidingSpring
10:30:19.34 +31:22:28.5 17.9mag 164P/Christensen
06:22:21.40 +24:28:14.9 17.9mag 198P/ODAS
15:04:59.30 -00:55:47.5 17.4mag 210P/Christensen
21:15:45.10 -13:18:13.0 17.5mag 218P/LINEAR
17:13:44.68 -14:49:57.3 16.2mag 235P/LINEAR
05:18:08.36 +34:03:30.7 16.6mag 240P/NEAT
07:35:02.24 -06:01:53.5 17.6mag 242P/Spahr
15:45:19.19 +06:27:49.6 17.5mag 391P/Kowalski
07:31:32.44 +21:19:40.6 17.6mag 450P/LONEOS
05:24:53.82 +45:29:00.2 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 03:06 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 03:06 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 03:06 tns_transients_list.txt
