This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AU Vul,2461144.8231,10.43,0.05,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
AU Vul 20260414.3231 10.43CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FY Cyg,2461144.8231,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FY Cyg 20260414.3231 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.1824+34.1798,2461144.8231,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.1824+34.1798 20260414.3231 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200500.42+282902.6,2461144.8231,12.82,0.05,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
ZTF J200500.42+282902.6 20260414.3231 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.7019+33.2446,2461144.8231,13.23,0.05,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
ATO J295.7019+33.2446 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1836678545783775872,2461144.8231,13.27,0.05,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
Gaia DR3 1836678545783775872 20260414.3231 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193822.53+293335.9,2461144.8231,12.86,0.05,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 J193822.53+293335.9 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201951.12+281329.2,2461144.8231,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201951.12+281329.2 20260414.3231 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201926.66+263646.3,2461144.8231,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201926.66+263646.3 20260414.3231 11.78CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GQ Vul,2461144.8231,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GQ Vul 20260414.3231 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1146 Cyg,2461144.8231,13.09,0.05,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
V1146 Cyg 20260414.3231 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195852.51+273248.7,2461144.8231,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195852.51+273248.7 20260414.3231 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200724.74+324515.6,2461144.8231,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200724.74+324515.6 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.8231,12.86,0.05,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
target 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200433.19+261340.3,2461144.8231,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200433.19+261340.3 20260414.3231 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1835646830238432640,2461144.8231,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835646830238432640 20260414.3231 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8367053,2461144.8231,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8367053 20260414.3231 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201952.79+321923.8,2461144.8231,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201952.79+321923.8 20260414.3231 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IO Cyg,2461144.8231,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IO Cyg 20260414.3231 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195550.51+300149.5,2461144.8231,12.51,0.05,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 J195550.51+300149.5 20260414.3231 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201342.77+295110.3,2461144.8231,12.87,0.05,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
ZTF J201342.77+295110.3 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201719.73+275006.8,2461144.8231,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201719.73+275006.8 20260414.3231 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8363904,2461144.8231,12.78,0.05,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 8363904 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201954.50+313719.7,2461144.8231,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201954.50+313719.7 20260414.3231 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201923.27+285932.0,2461144.8231,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201923.27+285932.0 20260414.3231 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.5730+26.4883,2461144.8231,12.82,0.05,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
ATO J302.5730+26.4883 20260414.3231 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FM Cyg,2461144.8231,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FM Cyg 20260414.3231 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-05667,2461144.8231,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05667 20260414.3231 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201730.60+262400.7,2461144.8231,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201730.60+262400.7 20260414.3231 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194502.04+291505.7,2461144.8231,12.87,0.05,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
ASASSN-V J194502.04+291505.7 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2920 Cyg,2461144.8231,12.26,0.05,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
V2920 Cyg 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8451676,2461144.8231,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8451676 20260414.3231 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201901.56+293446.7,2461144.8231,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201901.56+293446.7 20260414.3231 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201946.97+334022.4,2461144.8231,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201946.97+334022.4 20260414.3231 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2019134+264158,2461144.8231,11.26,0.05,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
NSVS J2019134+264158 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2053915659465816832,2461144.8231,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2053915659465816832 20260414.3231 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200720.94+284343.5,2461144.8231,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200720.94+284343.5 20260414.3231 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[WM2007] 1467,2461144.8231,13.12,0.05,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
[WM2007] 1467 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1836281763839484032,2461144.8231,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1836281763839484032 20260414.3231 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2029486126013515264,2461144.8231,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2029486126013515264 20260414.3231 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EV Cyg,2461144.8231,12.21,0.05,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
EV Cyg 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193813.04+294606.1,2461144.8231,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193813.04+294606.1 20260414.3231 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201913.34+321540.3,2461144.8231,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201913.34+321540.3 20260414.3231 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8545642,2461144.8231,13.05,0.05,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
NSVS 8545642 20260414.3231 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.8231,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.3231 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193741.73+283715.4,2461144.8231,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193741.73+283715.4 20260414.3231 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR2 1837066570311302784,2461144.8231,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR2 1837066570311302784 20260414.3231 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1837245107817975936,2461144.8231,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1837245107817975936 20260414.3231 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201456.38+273020.9,2461144.8231,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201456.38+273020.9 20260414.3231 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195253+2555.0,2461144.8231,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J195253+2555.0 20260414.3231 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461144.82347265 14.04.2026 07:45:38.037 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 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): 23127
Objects passed selection criteria: 23062
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 18968
Average stars matched: 18450.5 (97.2717 %)
Memory usage VmPeak: 129064 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 02:49:27 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461144.82347265 14.04.2026 07:45:38.037 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 287
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 78 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): 219199
Objects passed selection criteria: 218647
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 172558
Average stars matched: 166203 (96.317 %)
Memory usage VmPeak: 2051304 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 02:55:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461144.82279285
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:53.158 +30:00:20.77
Angular distance between the image centers 0.0282 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:50.512 +30:00:18.08
Angular distance between the image centers 0.0378 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:59:53.158 +30:00:20.77
Second-epoch second image center 19:59:50.512 +30:00:18.08
Angular distance between the image centers 0.00958 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.uzNdCXXxXF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.5EMSwPAGhH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits &> /tmp/tmp.SvZezkqGaU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits &> /tmp/tmp.xFlTxSW2IN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 30878 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2644 to 309.4609 deg, Dec +24.2020 to +35.3348 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 290.2644 to 309.4609 deg, Dec 24.2020 to 35.3348 deg
Loaded 30795 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6699 out of 7455 total matches.
Matched with Tycho-2 7455 out of 30878 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854269
a=0.000000 b=1.000000 c=22.854269
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
2.8 pix fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
2.8 pix fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Limiting magnitude estimates:
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.8 mag. fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
13.8 mag. fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uzNdCXXxXF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3756, passed=30878
Got 30878 stars (including 27089 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 30878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 631 matched stars entering correct_measured_positions(), 19509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 701 matched stars entering correct_measured_positions(), 19538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.51"
Accuracy estimation diagnostic: 698 matched stars entering correct_measured_positions(), 21385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.18"
Excluding outliers - 698 stars left (next iteration limit 694)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5EMSwPAGhH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3771, passed=30931
Got 30931 stars (including 27121 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 30931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 541 matched stars entering correct_measured_positions(), 474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.80"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 533 matched stars entering correct_measured_positions(), 15522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.95"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 585 matched stars entering correct_measured_positions(), 15534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.91"
Accuracy estimation diagnostic: 583 matched stars entering correct_measured_positions(), 16703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.33"
Excluding outliers - 583 stars left (next iteration limit 586)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SvZezkqGaU (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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=975, passed=14726
Got 14726 stars (including 13741 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat
util/solve_plate_with_UCAC5 got 14726 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 14218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 14219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 14219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.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.xFlTxSW2IN (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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=942, passed=14637
Got 14637 stars (including 13685 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat
util/solve_plate_with_UCAC5 got 14637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 14115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 14120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 14119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits'
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out06475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20398.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51980_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 51980_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:32:11.32 +27:37:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52033_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 52033_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:45:29.10 +31:26:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52058_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 52058_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:34:30.44 +27:34:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09276_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 09276_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:33:52.28 +28:19:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12059_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 12059_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:06.12 +29:45:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09275_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 09275_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:57.96 +28:30:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06475_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 06475_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20398_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 20398_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12413_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 12413_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:03:38.76 +29:53:34.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06526_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 06526_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:01:06.18 +27:45:16.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08725_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 08725_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:14:14.26 +28:41:41.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04508_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 04508_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:10:33.49 +26:54:17.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04231_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 04231_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:11:47.80 +26:48:34.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06428_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 06428_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:45.64 +27:48:53.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24893_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 24893_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:23.56 +33:43:39.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:18:05.64 +27:44:03.6
19:45:10.71 +32:03:08.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:53.158 +30:00:20.77
Angular distance between the image centers 0.0282 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:50.512 +30:00:18.08
Angular distance between the image centers 0.0378 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:59:53.158 +30:00:20.77
Second-epoch second image center 19:59:50.512 +30:00:18.08
Angular distance between the image centers 0.00958 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.YkZySDBEm2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.v38msXejeB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits &> /tmp/tmp.QlCXAyBH51
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits &> /tmp/tmp.Q1TUMZbjIP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 281578 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2219 to 309.4679 deg, Dec +24.1963 to +35.3349 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 290.2219 to 309.4679 deg, Dec 24.1963 to 35.3349 deg
Loaded 30877 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5684 out of 8842 total matches.
Matched with Tycho-2 8842 out of 281578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629178
a=0.000000 b=1.000000 c=22.629178
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 197 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
2.6 pix fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
2.6 pix fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Limiting magnitude estimates:
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.9 mag. fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
13.8 mag. fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (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.YkZySDBEm2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=51531, passed=281520
Got 281520 stars (including 229582 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 281520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 642 matched stars entering correct_measured_positions(), 589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.01"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 635 matched stars entering correct_measured_positions(), 211069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 754 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 715 matched stars entering correct_measured_positions(), 211109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
Accuracy estimation diagnostic: 713 matched stars entering correct_measured_positions(), 228657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Excluding outliers - 713 stars left (next iteration limit 698)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.v38msXejeB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=51082, passed=280646
Got 280646 stars (including 229187 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 280646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 584 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 520 matched stars entering correct_measured_positions(), 457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 517 matched stars entering correct_measured_positions(), 153986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 154010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 174936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 567 stars left (next iteration limit 568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QlCXAyBH51 (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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=12841, passed=112637
Got 112637 stars (including 99687 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat
util/solve_plate_with_UCAC5 got 112637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 109761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 109765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 109765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.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.Q1TUMZbjIP (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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=12961, passed=112839
Got 112839 stars (including 99784 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat
util/solve_plate_with_UCAC5 got 112839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 109781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 109782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 109779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-44-39_20.00sec_-4.90C_LIGHT_0850.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.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_2026-04-14_CI_Cyg-08-Q2b1x1_024628_TTUQ2b1x1_9010_z3Hqw5yl/wcs_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851.fits
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out315801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94562.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 38s
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: 23s
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Considering the candidate 315801_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315801_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:00:28.57 +27:52:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 315802_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315802_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:01.25 +31:04:14.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 315809_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315809_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:57:20.74 +31:28:46.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 315813_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315813_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:40:30.52 +31:29:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315823_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315823_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:49:01.42 +31:46:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315830_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315830_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:29.59 +31:32:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315832_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315832_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:48.22 +33:40:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
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Considering the candidate 315835_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315835_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:09:37.02 +33:42:24.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 315837_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315837_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:36:59.72 +31:00:57.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 315849_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315849_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:54:41.57 +33:02:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315860_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 315860_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 315868_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315868_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:49.94 +32:06:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315869_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 315869_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 315873_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315873_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:48:07.82 +29:51:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315874_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315874_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:10:08.88 +25:54:47.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 315875_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315875_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:12:45.59 +34:12:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 5.515 2055669513640230400 303.19180752887 +34.20575704697 12.6207 12.1410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315876_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315876_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:41.12 +32:47:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 315884_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315884_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:08:40.95 +32:24:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.616 2054892541182602368 302.17046754946 +32.41695641457 12.3597 11.0670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 315898_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315898_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:04:34.27 +33:27:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315904_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315904_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:43:59.46 +30:12:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315905_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315905_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:39:34.16 +31:04:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315917_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315917_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:54:06.17 +33:48:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315918_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315918_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:28:39.23 +31:20:45.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 315948_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315948_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:30:39.83 +27:54:38.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 315994_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 315994_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:45:29.06 +31:26:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316039_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316039_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:31:48.60 +33:23:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316091_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316091_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:33:04.65 +27:22:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316128_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316128_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:37:06.12 +28:11:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316140_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316140_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:06:56.21 +33:18:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316173_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316173_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:14:18.44 +28:40:30.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316187_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316187_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:44:46.85 +29:14:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316190_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316190_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:37:25.58 +29:37:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316196_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316196_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:29:32.77 +31:21:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316198_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316198_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:59:40.74 +32:01:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.320 2033980998282503296 299.91999071127 +32.02063911954 11.2746 9.7198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316199_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316199_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:25.77 +33:53:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316201_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316201_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:48:57.24 +33:25:49.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316207_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316207_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:37:05.32 +28:12:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316211_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316211_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:45:30.32 +33:37:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316224_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316224_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:35:18.29 +27:52:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316231_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316231_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:40:09.15 +26:59:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316244_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316244_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:30:12.74 +33:44:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316273_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316273_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:49:50.56 +28:27:42.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316283_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316283_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:44:26.90 +33:59:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.727 2047055394120738176 296.11171792533 +33.98291697443 13.1977 12.4417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316288_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316288_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:37:09.46 +28:28:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:48:42.48 +33:25:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316296_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316296_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:14:42.19 +26:25:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316299_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316299_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:32:07.21 +28:15:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316303_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316303_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:40:29.85 +34:04:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316308_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316308_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:31:39.66 +26:58:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316311_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316311_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:56:39.59 +30:58:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316324_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316324_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:39.97 +32:55:54.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 316330_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316330_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:08.65 +29:40:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316333_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316333_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:49:51.12 +27:06:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316336_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316336_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:36:35.46 +31:17:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316337_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316337_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:02.42 +27:05:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316345_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316345_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 316351_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316351_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 316356_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316356_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:32:50.07 +31:41:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316359_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316359_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:40:29.61 +31:16:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316361_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316361_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:31:10.18 +33:27:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316374_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316374_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:52:55.42 +28:59:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316385_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316385_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:00:02.25 +25:58:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316387_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316387_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:34:29.08 +29:37:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316398_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316398_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:30.97 +33:42:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316402_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316402_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:41:17.44 +30:39:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316403_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316403_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:53.25 +27:02:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316419_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316419_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:10:07.32 +26:18:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.891 1836358179897198464 302.53159834808 +26.30566792253 12.3321 11.0224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316420_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316420_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:36:27.99 +31:13:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316421_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316421_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:59:05.15 +33:20:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316424_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316424_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:50.65 +27:40:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316426_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316426_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:43:08.88 +29:41:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.312 2031990912266643584 295.78739546694 +29.68637597543 13.3161 12.4987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316427_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316427_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:43:27.99 +27:49:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.766 2031167584218814720 295.86548776609 +27.82628743063 12.1972 10.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316433_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316433_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:52:24.14 +25:56:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316441_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316441_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:11:30.94 +29:10:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316460_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316460_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:23.40 +32:45:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316462_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316462_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:55.04 +34:07:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316476_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316476_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:30:05.71 +33:52:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316482_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 316482_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 316487_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316487_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:48:57.83 +31:18:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316490_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316490_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:36:01.31 +29:51:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316510_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316510_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:39:25.27 +29:56:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316514_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316514_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:05:23.72 +31:58:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316518_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316518_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:54:58.04 +33:08:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316522_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316522_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:51:15.65 +26:35:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316526_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316526_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:50:39.80 +27:25:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.938 2027952822702827520 297.66563833885 +27.42288932520 11.0997 9.6050 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316551_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316551_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:43.76 +33:18:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316553_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316553_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:53:18.62 +28:24:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316569_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316569_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:45:49.04 +33:55:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316598_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316598_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:49:37.38 +29:22:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316600_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316600_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:50.43 +32:41:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316613_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316613_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:43:52.35 +33:54:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316620_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316620_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:26.17 +27:51:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316659_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316659_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:05:18.05 +33:28:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316675_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316675_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:48:32.27 +32:06:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316680_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 316680_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:51:28.62 +32:47:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109075_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 109075_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:29:15.88 +28:54:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298383_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 298383_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:30:20.70 +30:54:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48660_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 48660_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 123987_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 123987_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 124027_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 124027_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:02:29.67 +29:51:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 313682_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 313682_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:02:12.82 +30:57:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72337_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 72337_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 35292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 35292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 27053_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 27053_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 114440_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 114440_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:12:57.92 +29:38:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104878_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 104878_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:02:11.97 +29:13:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 82746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 57703_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 57703_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 120106_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 120106_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:06.01 +29:45:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110658_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 110658_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:52:10.38 +29:21:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211187_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 211187_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 21914_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 21914_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:17:43.08 +25:57:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111422_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 111422_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:45.67 +29:24:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20441_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 20441_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 49137_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 49137_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:51:01.61 +27:04:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28254_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 28254_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 25950_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 25950_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 37216_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 37216_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 199052_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 199052_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 31831_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 31831_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:14:35.19 +26:27:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210789_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 210789_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 130933_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 130933_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 166201_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 166201_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:04:45.67 +31:12:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 121292_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 87644_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 87644_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:25.13 +28:44:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62278_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 62278_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 43550_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 43550_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 178135_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 178135_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 94562_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 94562_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 217695_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 217695_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:27.81 +32:53:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 281000_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 281000_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:54:23.65 +34:04:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208479_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 208479_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:55:32.34 +32:33:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32904_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 32904_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 142941_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 142941_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 242176_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 242176_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 25199_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 25199_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:07.57 +26:07:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161186_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 161186_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:20:03.13 +31:04:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 42746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:53:46.33 +26:49:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30822_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 30822_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 119004_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 119004_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:58:13.97 +29:41:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110408_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 110408_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 202270_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 202270_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 202882_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 202882_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 155851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 155851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:58:22.92 +30:49:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113931_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 113931_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 80945_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 80945_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:56.13 +28:32:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160448_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 160448_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:37.23 +31:01:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243527_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 243527_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 38638_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 38638_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 73692_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 73692_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:49:26.74 +28:05:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 184746_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 189527_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 189527_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:09:43.59 +31:59:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87433_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 87433_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 246966_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 246966_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:44:24.91 +33:18:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70730_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 70730_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 62123_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 62123_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 107506_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 107506_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 68455_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 68455_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:32:09.04 +27:33:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119858_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 119858_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 127236_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 127236_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:03:09.95 +29:59:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95893_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 95893_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:33:33.02 +28:33:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102097_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 102097_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:42:35.24 +28:56:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296366_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 296366_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:49.76 +32:24:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134579_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 134579_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:04.24 +30:14:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34870_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 34870_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:59:29.19 +26:30:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 130851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
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Considering the candidate 197262_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 197262_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80414_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 80414_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295549_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 295549_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295444_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 295444_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:16:18.53 +28:48:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295291_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 295291_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72500_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 72500_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83979_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 83979_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60401_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 60401_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:05.75 +27:44:03.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97966_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 97966_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:38:57.98 +28:30:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 149851_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:45.76 +30:43:56.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54677_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 54677_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186339_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 186339_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:20:28.66 +31:53:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24692_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
Preparing report for the candidate 24692_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43055_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 43055_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:47:37.09 +26:45:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46374_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 46374_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:07:07.31 +27:06:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131640_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 131640_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:59:12.56 +30:05:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90024_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 90024_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:33:52.28 +28:19:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170841_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 170841_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:20:18.40 +31:23:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198834_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 198834_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:45:10.69 +32:03:08.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127342_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 127342_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:03:38.77 +29:53:34.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165195_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 165195_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 19:58:38.17 +30:58:59.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65096_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 65096_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:01:06.19 +27:45:16.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200287_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 200287_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:04:36.01 +32:13:01.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102040_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 102040_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:17:31.46 +29:08:51.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89079_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 89079_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:14:14.31 +28:41:42.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44319_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 44319_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:10:33.50 +26:54:16.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65977_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 65977_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:45.62 +27:48:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41894_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 41894_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:11:47.84 +26:48:34.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34195_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 34195_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:12:00.69 +26:28:43.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45279_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 45279_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:18:50.54 +26:59:28.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241308_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851
The candidate 241308_fd_Cyg-08-Q2b1x1_2026-04-14_02-45-38_20.00sec_-4.90C_LIGHT_0851 did not pass the final checks
**** FOUND 20:15:23.56 +33:43:38.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 64s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:18:05.64 +27:44:03.6
19:45:10.71 +32:03:08.3
20:11:37.35 +29:24:33.2
19:45:02.23 +29:15:00.4
20:19:01.27 +29:34:47.5
19:53:01.87 +29:38:55.6
20:13:42.61 +29:51:09.7
19:38:22.46 +29:33:33.9
19:38:13.12 +29:46:10.7
19:55:50.66 +30:01:48.7
19:30:07.74 +29:55:15.8
20:19:54.21 +31:37:17.8
20:17:42.71 +31:50:49.3
20:19:13.03 +32:15:38.2
20:19:52.43 +32:19:19.1
20:20:31.46 +32:26:45.6
19:56:37.45 +32:22:09.1
20:18:23.57 +25:52:54.2
19:44:34.52 +32:29:10.8
20:07:24.69 +32:45:12.6
19:49:50.48 +33:33:35.6
20:19:46.65 +33:40:18.2
19:52:52.66 +25:54:59.7
20:14:46.88 +26:10:21.7
19:47:58.10 +26:00:02.0
20:04:33.03 +26:13:41.0
19:37:42.32 +28:37:14.8
20:18:02.92 +28:06:15.3
20:17:30.30 +26:24:02.2
20:16:43.28 +34:10:45.4
20:05:01.45 +28:29:19.5
19:42:48.01 +33:14:22.9
20:10:17.31 +26:29:21.6
20:19:26.36 +26:36:47.7
19:32:36.28 +26:12:15.9
20:19:13.09 +26:41:59.1
19:30:11.15 +26:28:04.8
20:07:06.94 +27:12:43.2
20:14:56.20 +27:30:21.7
19:58:52.78 +27:32:53.3
20:20:07.49 +27:50:24.9
20:17:19.42 +27:50:07.5
20:02:59.92 +28:07:00.4
20:19:50.70 +28:13:29.6
20:17:18.68 +28:14:21.0
20:19:25.12 +28:31:43.7
19:44:12.01 +28:19:21.5
20:12:46.15 +28:38:07.6
20:07:20.80 +28:43:44.5
20:19:22.94 +28:59:32.1
########### Completed Cyg-08-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:18:05.64 +27:44:03.6
19:45:10.71 +32:03:08.3
20:16:43.28 +34:10:45.4
20:05:01.45 +28:29:19.5
19:42:48.01 +33:14:22.9
20:07:06.94 +27:12:43.2
19:38:22.46 +29:33:33.9
20:19:50.70 +28:13:29.6
20:19:26.36 +26:36:47.7
19:47:58.10 +26:00:02.0
19:44:12.01 +28:19:21.5
19:58:52.78 +27:32:53.3
20:07:24.69 +32:45:12.6
20:18:23.57 +25:52:54.2
20:04:33.03 +26:13:41.0
20:14:46.88 +26:10:21.7
19:32:36.28 +26:12:15.9
20:19:52.43 +32:19:19.1
19:44:34.52 +32:29:10.8
19:55:50.66 +30:01:48.7
20:13:42.61 +29:51:09.7
20:17:19.42 +27:50:07.5
19:30:11.15 +26:28:04.8
20:19:54.21 +31:37:17.8
20:19:22.94 +28:59:32.1
20:10:17.31 +26:29:21.6
19:30:07.74 +29:55:15.8
19:49:50.48 +33:33:35.6
20:17:30.30 +26:24:02.2
19:45:02.23 +29:15:00.4
20:20:31.46 +32:26:45.6
19:56:37.45 +32:22:09.1
20:19:01.27 +29:34:47.5
20:19:46.65 +33:40:18.2
20:19:13.09 +26:41:59.1
20:17:42.71 +31:50:49.3
20:07:20.80 +28:43:44.5
20:02:59.92 +28:07:00.4
20:20:07.49 +27:50:24.9
20:11:37.35 +29:24:33.2
19:53:01.87 +29:38:55.6
19:38:13.12 +29:46:10.7
20:19:13.03 +32:15:38.2
20:19:25.12 +28:31:43.7
20:18:02.92 +28:06:15.3
19:37:42.32 +28:37:14.8
20:17:18.68 +28:14:21.0
20:12:46.15 +28:38:07.6
20:14:56.20 +27:30:21.7
19:52:52.66 +25:54:59.7
###################################################################################
20:18:05.64 +27:44:03.6 -- not an asteroid (will add it to exclusion list)
19:45:10.71 +32:03:08.3 -- not an asteroid (will add it to exclusion list)
20:16:43.28 +34:10:45.4 -- not an asteroid (will add it to exclusion list)
20:05:01.45 +28:29:19.5 -- not an asteroid (will add it to exclusion list)
19:42:48.01 +33:14:22.9 -- not an asteroid (will add it to exclusion list)
20:07:06.94 +27:12:43.2 -- not an asteroid (will add it to exclusion list)
19:38:22.46 +29:33:33.9 -- not an asteroid (will add it to exclusion list)
20:19:50.70 +28:13:29.6 -- not an asteroid (will add it to exclusion list)
20:19:26.36 +26:36:47.7 -- not an asteroid (will add it to exclusion list)
19:47:58.10 +26:00:02.0 -- not an asteroid (will add it to exclusion list)
19:44:12.01 +28:19:21.5 -- not an asteroid (will add it to exclusion list)
19:58:52.78 +27:32:53.3 -- not an asteroid (will add it to exclusion list)
20:07:24.69 +32:45:12.6 -- not an asteroid (will add it to exclusion list)
20:18:23.57 +25:52:54.2 -- not an asteroid (will add it to exclusion list)
20:04:33.03 +26:13:41.0 -- not an asteroid (will add it to exclusion list)
20:14:46.88 +26:10:21.7 -- not an asteroid (will add it to exclusion list)
19:32:36.28 +26:12:15.9 -- not an asteroid (will add it to exclusion list)
20:19:52.43 +32:19:19.1 -- not an asteroid (will add it to exclusion list)
19:44:34.52 +32:29:10.8 -- not an asteroid (will add it to exclusion list)
19:55:50.66 +30:01:48.7 -- not an asteroid (will add it to exclusion list)
20:13:42.61 +29:51:09.7 -- not an asteroid (will add it to exclusion list)
20:17:19.42 +27:50:07.5 -- not an asteroid (will add it to exclusion list)
19:30:11.15 +26:28:04.8 -- not an asteroid (will add it to exclusion list)
20:19:54.21 +31:37:17.8 -- not an asteroid (will add it to exclusion list)
20:19:22.94 +28:59:32.1 -- not an asteroid (will add it to exclusion list)
20:10:17.31 +26:29:21.6 -- not an asteroid (will add it to exclusion list)
19:30:07.74 +29:55:15.8 -- not an asteroid (will add it to exclusion list)
19:49:50.48 +33:33:35.6 -- not an asteroid (will add it to exclusion list)
20:17:30.30 +26:24:02.2 -- not an asteroid (will add it to exclusion list)
19:45:02.23 +29:15:00.4 -- not an asteroid (will add it to exclusion list)
20:20:31.46 +32:26:45.6 -- not an asteroid (will add it to exclusion list)
19:56:37.45 +32:22:09.1 -- not an asteroid (will add it to exclusion list)
20:19:01.27 +29:34:47.5 -- not an asteroid (will add it to exclusion list)
20:19:46.65 +33:40:18.2 -- not an asteroid (will add it to exclusion list)
20:19:13.09 +26:41:59.1 -- not an asteroid (will add it to exclusion list)
20:17:42.71 +31:50:49.3 -- not an asteroid (will add it to exclusion list)
20:07:20.80 +28:43:44.5 -- not an asteroid (will add it to exclusion list)
20:02:59.92 +28:07:00.4 -- not an asteroid (will add it to exclusion list)
20:20:07.49 +27:50:24.9 -- not an asteroid (will add it to exclusion list)
20:11:37.35 +29:24:33.2 -- not an asteroid (will add it to exclusion list)
19:53:01.87 +29:38:55.6 -- not an asteroid (will add it to exclusion list)
19:38:13.12 +29:46:10.7 -- not an asteroid (will add it to exclusion list)
20:19:13.03 +32:15:38.2 -- not an asteroid (will add it to exclusion list)
20:19:25.12 +28:31:43.7 -- not an asteroid (will add it to exclusion list)
20:18:02.92 +28:06:15.3 -- not an asteroid (will add it to exclusion list)
19:37:42.32 +28:37:14.8 -- not an asteroid (will add it to exclusion list)
20:17:18.68 +28:14:21.0 -- not an asteroid (will add it to exclusion list)
20:12:46.15 +28:38:07.6 -- not an asteroid (will add it to exclusion list)
20:14:56.20 +27:30:21.7 -- not an asteroid (will add it to exclusion list)
19:52:52.66 +25:54:59.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:30:07.74 +29:55:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:11.15 +26:28:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:36.28 +26:12:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:42.32 +28:37:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:13.12 +29:46:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:22.46 +29:33:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:48.01 +33:14:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:12.01 +28:19:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:34.52 +32:29:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:02.23 +29:15:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:10.71 +32:03:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:58.10 +26:00:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:50.48 +33:33:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:52.66 +25:54:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:01.87 +29:38:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:50.66 +30:01:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:37.45 +32:22:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:52.78 +27:32:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:59.92 +28:07:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:33.03 +26:13:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:01.45 +28:29:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:06.94 +27:12:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:20.80 +28:43:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:24.69 +32:45:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:17.31 +26:29:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:37.35 +29:24:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:46.15 +28:38:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:42.61 +29:51:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:46.88 +26:10:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:56.20 +27:30:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:43.28 +34:10:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:18.68 +28:14:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:19.42 +27:50:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:30.30 +26:24:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:42.71 +31:50:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:02.92 +28:06:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:05.64 +27:44:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:23.57 +25:52:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:01.27 +29:34:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:13.03 +32:15:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:13.09 +26:41:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:22.94 +28:59:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:25.12 +28:31:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:26.36 +26:36:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:46.65 +33:40:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:50.70 +28:13:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:52.43 +32:19:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:54.21 +31:37:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:07.49 +27:50:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:31.46 +32:26:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:30:07.74 +29:55:15.8 -- a known variable star
19:30:11.15 +26:28:04.8 -- a known variable star
19:32:36.28 +26:12:15.9 -- a known variable star
19:37:42.32 +28:37:14.8 -- a known variable star
19:38:13.12 +29:46:10.7 -- a known variable star
19:38:22.46 +29:33:33.9 -- a known variable star
19:42:48.01 +33:14:22.9 -- not a known variable star
19:44:12.01 +28:19:21.5 -- a known variable star
19:44:34.52 +32:29:10.8 -- a known variable star
19:45:02.23 +29:15:00.4 -- a known variable star
19:45:10.71 +32:03:08.3 -- a known variable star
19:47:58.10 +26:00:02.0 -- a known variable star
19:49:50.48 +33:33:35.6 -- a known variable star
19:52:52.66 +25:54:59.7 -- a known variable star
19:53:01.87 +29:38:55.6 -- a known variable star
19:55:50.66 +30:01:48.7 -- a known variable star
19:56:37.45 +32:22:09.1 -- a known variable star
19:58:52.78 +27:32:53.3 -- a known variable star
20:02:59.92 +28:07:00.4 -- a known variable star
20:04:33.03 +26:13:41.0 -- a known variable star
20:05:01.45 +28:29:19.5 -- a known variable star
20:07:06.94 +27:12:43.2 -- not a known variable star
20:07:20.80 +28:43:44.5 -- a known variable star
20:07:24.69 +32:45:12.6 -- a known variable star
20:10:17.31 +26:29:21.6 -- not a known variable star
20:11:37.35 +29:24:33.2 -- a known variable star
20:12:46.15 +28:38:07.6 -- a known variable star
20:13:42.61 +29:51:09.7 -- a known variable star
20:14:46.88 +26:10:21.7 -- a known variable star
20:14:56.20 +27:30:21.7 -- a known variable star
20:16:43.28 +34:10:45.4 -- not a known variable star
20:17:18.68 +28:14:21.0 -- a known variable star
20:17:19.42 +27:50:07.5 -- a known variable star
20:17:30.30 +26:24:02.2 -- a known variable star
20:17:42.71 +31:50:49.3 -- a known variable star
20:18:02.92 +28:06:15.3 -- not a known variable star
20:18:05.64 +27:44:03.6 -- a known variable star
20:18:23.57 +25:52:54.2 -- not a known variable star
20:19:01.27 +29:34:47.5 -- a known variable star
20:19:13.03 +32:15:38.2 -- a known variable star
20:19:13.09 +26:41:59.1 -- a known variable star
20:19:22.94 +28:59:32.1 -- a known variable star
20:19:25.12 +28:31:43.7 -- a known variable star
20:19:26.36 +26:36:47.7 -- a known variable star
20:19:46.65 +33:40:18.2 -- a known variable star
20:19:50.70 +28:13:29.6 -- a known variable star
20:19:52.43 +32:19:19.1 -- a known variable star
20:19:54.21 +31:37:17.8 -- a known variable star
20:20:07.49 +27:50:24.9 -- a known variable star
20:20:31.46 +32:26:45.6 -- a known variable star
Found 6 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
50 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:30:07.74 +29:55:15.8
19:30:11.15 +26:28:04.8
19:32:36.28 +26:12:15.9
19:37:42.32 +28:37:14.8
19:38:13.12 +29:46:10.7
19:38:22.46 +29:33:33.9
19:42:48.01 +33:14:22.9
19:44:12.01 +28:19:21.5
19:44:34.52 +32:29:10.8
19:45:02.23 +29:15:00.4
19:45:10.71 +32:03:08.3
19:47:58.10 +26:00:02.0
19:49:50.48 +33:33:35.6
19:52:52.66 +25:54:59.7
19:53:01.87 +29:38:55.6
19:55:50.66 +30:01:48.7
19:56:37.45 +32:22:09.1
19:58:52.78 +27:32:53.3
20:02:59.92 +28:07:00.4
20:04:33.03 +26:13:41.0
20:05:01.45 +28:29:19.5
20:07:06.94 +27:12:43.2
20:07:20.80 +28:43:44.5
20:07:24.69 +32:45:12.6
20:10:17.31 +26:29:21.6
20:11:37.35 +29:24:33.2
20:12:46.15 +28:38:07.6
20:13:42.61 +29:51:09.7
20:14:46.88 +26:10:21.7
20:14:56.20 +27:30:21.7
20:16:43.28 +34:10:45.4
20:17:18.68 +28:14:21.0
20:17:19.42 +27:50:07.5
20:17:30.30 +26:24:02.2
20:17:42.71 +31:50:49.3
20:18:02.92 +28:06:15.3
20:18:05.64 +27:44:03.6
20:18:23.57 +25:52:54.2
20:19:01.27 +29:34:47.5
20:19:13.03 +32:15:38.2
20:19:13.09 +26:41:59.1
20:19:22.94 +28:59:32.1
20:19:25.12 +28:31:43.7
20:19:26.36 +26:36:47.7
20:19:46.65 +33:40:18.2
20:19:50.70 +28:13:29.6
20:19:52.43 +32:19:19.1
20:19:54.21 +31:37:17.8
20:20:07.49 +27:50:24.9
20:20:31.46 +32:26:45.6
20:00:28.57 +27:52:09.1
19:50:01.25 +31:04:14.6
19:57:20.74 +31:28:46.6
20:16:48.22 +33:40:46.7
20:09:37.02 +33:42:24.8
19:36:59.72 +31:00:57.9
20:10:08.88 +25:54:47.7
20:12:45.59 +34:12:20.4
20:18:41.12 +32:47:16.1
20:08:40.95 +32:24:59.5
19:59:40.74 +32:01:12.1
19:44:26.90 +33:59:01.0
20:10:07.32 +26:18:18.8
19:43:08.88 +29:41:09.0
19:43:27.99 +27:49:33.6
19:50:39.80 +27:25:21.7
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461144.82279285 -observatory V36
23:58:33.52 -02:57:23.7 Mercury (0.1mag)
03:00:28.07 +17:13:07.4 Venus (-3.9mag)
00:13:04.76 +00:20:25.1 Mars (1.2mag)
07:11:52.93 +22:47:26.7 Jupiter (-2.1mag)
00:28:25.99 +00:44:18.5 Saturn (0.9mag)
03:47:20.76 +19:46:20.9 Uranus (5.8mag)
00:10:37.22 -00:16:45.6 Neptune (7.8mag)
20:33:40.75 -22:52:31.8 Pluto (14.5mag)
22:56:24.78 -07:02:31.8 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Apr 14 02:49 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.82279285:
07:11:53.57 +22:47:27.9 Io (5.8mag)
07:11:48.39 +22:47:33.4 Europa (5.9mag)
07:12:03.79 +22:47:10.3 Ganymede (5.3mag)
07:12:20.57 +22:46:36.8 Callisto (6.6mag)
07:15:17.55 +22:35:51.4 Himalia (15.3mag)
07:11:51.37 +22:47:32.0 Thebe (16.2mag)
07:15:26.74 +23:05:55.0 Elara (17.3mag)
07:10:38.99 +23:28:19.6 Pasiphae (17.4mag)
07:20:14.87 +22:45:17.9 Carme (18.5mag)
00:28:33.49 +00:44:35.7 Titan (8.8mag)
00:28:27.13 +00:44:33.4 Rhea (10.1mag)
00:28:09.02 +00:44:44.0 Iapetus (11.5mag)
00:28:38.98 +00:44:28.3 Hyperion (14.8mag)
00:30:04.22 +00:53:17.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 14 02:49 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.82279285:
15:30:16.64 -15:05:23.3 JWST
17:18:43.38 +43:05:58.6 Chandra
08:27:50.57 -46:16:58.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 14 02:49 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.82279285 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:18.06 -28:40:53.4 13.9mag P/2010 H2 (Vales)
05:05:32.31 -69:44:29.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:05.29 +31:25:33.6 17.2mag C/2017 K2 (PANSTARRS)
17:30:35.50 +10:20:55.6 17.6mag C/2021 G2 (ATLAS)
23:09:46.47 +29:09:46.3 17.1mag C/2022 E2 (ATLAS)
04:27:17.12 +25:59:33.6 16.0mag C/2022 N2 (PANSTARRS)
09:03:04.15 +32:00:24.2 16.2mag C/2022 QE78 (ATLAS)
08:30:49.33 -00:19:53.0 17.3mag C/2022 R6 (PANSTARRS)
18:54:07.29 +18:23:29.3 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:12.68 -11:32:46.2 17.5mag P/2023 B1 (PANSTARRS)
09:08:25.36 -12:09:09.3 17.6mag C/2023 F3 (ATLAS)
21:52:31.10 +62:48:32.1 17.5mag C/2023 H5 (Lemmon)
19:20:37.55 -03:42:20.4 14.2mag C/2023 R1 (PANSTARRS)
21:35:39.78 +85:40:47.5 17.8mag C/2023 X2 (Lemmon)
06:17:08.17 +63:31:14.0 17.1mag C/2024 A1 (ATLAS)
05:09:39.44 +17:44:27.4 10.9mag C/2024 E1 (Wierzchos)
16:20:20.79 +06:06:55.9 17.4mag C/2024 G6 (ATLAS)
20:20:20.06 +14:49:12.4 14.6mag C/2024 J3 (ATLAS)
03:24:51.96 -22:38:29.1 16.4mag C/2024 T5 (ATLAS)
05:15:17.65 +45:42:31.9 17.7mag C/2025 J1 (Borisov)
13:45:47.96 +44:21:44.2 15.1mag C/2025 L1 (ATLAS)
03:22:38.12 -25:57:03.1 17.8mag C/2025 Q3 (ATLAS)
23:29:51.30 +19:06:25.5 8.8mag C/2025 R3 (PANSTARRS)
12:54:50.66 +02:54:37.6 17.4mag C/2025 Y1 (ATLAS)
03:13:33.57 +02:48:54.4 12.8mag C/2026 A1 (MAPS)
23:54:48.62 +36:54:28.4 14.5mag C/2026 B2 (Sun-Gao)
18:39:40.27 -09:48:32.2 11.9mag 10P/Tempel
15:02:33.91 +03:22:55.2 13.8mag 24P/Schaumasse
11:03:15.30 -01:34:49.8 15.7mag 29P/Schwassmann-Wachmann
18:00:27.33 -09:40:20.5 17.9mag 40P/Vaisala
10:37:38.73 -04:13:59.7 16.9mag 43P/Wolf-Harrington
01:46:04.73 +17:12:05.3 17.2mag 47P/Ashbrook-Jackson
07:07:40.54 +37:22:20.2 17.0mag 63P/Wild
23:26:54.99 -11:39:09.6 15.7mag 65P/Gunn
03:58:46.62 +20:40:34.4 15.9mag 76P/West-Kohoutek-Ikemura
01:01:52.22 +07:53:56.0 14.3mag 78P/Gehrels
22:57:54.99 -09:53:13.8 14.6mag 88P/Howell
02:05:39.72 +20:11:38.4 15.1mag 93P/Lovas
04:51:39.00 +32:11:51.4 16.2mag 123P/West-Hartley
08:26:23.98 +39:08:04.2 16.2mag 124P/Mrkos
02:30:37.56 +14:10:57.5 16.4mag 128P/Shoemaker-Holt
02:44:14.92 +14:17:16.8 17.5mag 131P/Mueller
01:17:22.29 +12:39:17.2 10.7mag 141P/Machholz
01:26:31.87 +04:14:39.0 10.7mag 141P-A/Machholz
00:12:38.42 +00:12:58.3 13.0mag 141P-D/Machholz
01:56:42.90 +05:59:51.9 17.8mag 141P-I/Machholz
00:57:42.21 -02:22:09.5 15.1mag 162P/SidingSpring
10:29:04.58 +30:56:43.4 18.0mag 164P/Christensen
06:33:25.86 +24:17:38.7 18.0mag 198P/ODAS
14:54:24.74 -00:14:34.4 17.6mag 210P/Christensen
21:33:58.52 -11:51:11.6 17.6mag 218P/LINEAR
17:16:07.33 -14:08:05.1 16.1mag 235P/LINEAR
05:30:51.79 +34:34:12.2 16.7mag 240P/NEAT
07:37:40.51 -05:20:58.2 17.7mag 242P/Spahr
22:12:43.15 -21:25:26.9 17.9mag 260P/McNaught
15:43:17.44 +06:52:46.1 17.5mag 391P/Kowalski
07:33:33.46 +21:21:37.6 17.7mag 450P/LONEOS
05:33:25.68 +45:07:50.2 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 14 02:49 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
-rw-r--r-- 1 apache apache 5.8K Apr 14 02:49 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 14 02:49 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:08:01.002 +67:05:08.73 AT 2026ivq 2026-04-04.49 19.4548
18:36:22.696 +81:45:06.35 AT 2026ivp 2026-03-27.51 20.7475
15:19:48.489 -05:00:11.22 AT 2026ivo 2026-03-27.48 21.2654
15:56:56.656 +27:09:01.74 AT 2026ivn 2026-04-04.38 19.6722
13:56:43.855 -19:49:48.79 AT 2026ivm 2026-04-07.40 19.7776
09:53:53.828 +01:43:05.64 AT 2026ivl 2026-04-07.17 22.04
11:56:09.924 +23:56:19.29 AT 2026ivk 2026-04-07.91 18.97
09:57:07.898 +44:06:56.68 AT 2026ivj 2026-03-30.18 19.5868
11:56:46.937 +30:48:49.43 AT 2026ivi 2026-04-07.29 20.1063
12:16:21.919 +30:21:04.60 AT 2026ivh 2026-04-07.29 19.651
09:11:45.682 +30:03:32.51 AT 2026ivg 2026-04-04.17 19.5142
09:55:25.809 -27:42:27.02 AT 2026ivf 2026-04-08.21 18.51
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
-rw-r--r-- 1 apache apache 30K Apr 14 02:49 tns_transients_list.txt
