This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz
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
CT Cep,2461140.9278,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CT Cep 20260410.4278 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0567 Cep,2461140.9278,11.07,0.05,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
V0567 Cep 20260410.4278 11.07CV 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
BI Cep,2461140.9278,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BI Cep 20260410.4278 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0579 Cep,2461140.9278,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0579 Cep 20260410.4278 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2219784444566102784,2461140.9278,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2219784444566102784 20260410.4278 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.9278,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.4278 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.9278,14.57,0.05,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
target 20260410.4278 14.57CV 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
ASASSN-V J215453.45+721041.9,2461140.9278,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215453.45+721041.9 20260410.4278 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0492 Cep,2461140.9278,13.46,0.05,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
V0492 Cep 20260410.4278 13.46CV 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
V0598 Cep,2461140.9278,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0598 Cep 20260410.4278 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Cep,2461140.9278,11.11,0.05,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
BM Cep 20260410.4278 11.11CV 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
NSVS 3395915,2461140.9278,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3395915 20260410.4278 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2104157+674246,2461140.9278,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2104157+674246 20260410.4278 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J222333.29+680434.4,2461140.9278,12.88,0.05,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
ASASSN-V J222333.29+680434.4 20260410.4278 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 J2219520+720116,2461140.9278,12.86,0.05,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
NSVS J2219520+720116 20260410.4278 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
NSVS J2056120+733332,2461140.9278,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2056120+733332 20260410.4278 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3382200,2461140.9278,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3382200 20260410.4278 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0858 Cep,2461140.9278,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0858 Cep 20260410.4278 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J220548.56+732903.2,2461140.9278,12.87,0.05,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 J220548.56+732903.2 20260410.4278 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 J221745.26+664612.9,2461140.9278,12.01,0.05,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
ASASSN-V J221745.26+664612.9 20260410.4278 12.01CV 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
NSVS J2147365+662832,2461140.9278,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2147365+662832 20260410.4278 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0634 Cep,2461140.9278,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0634 Cep 20260410.4278 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213319.60+654325.1,2461140.9278,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213319.60+654325.1 20260410.4278 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2113202+702404,2461140.9278,13.46,0.05,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
NSVS J2113202+702404 20260410.4278 13.46CV 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
NSVS J2151128+675611,2461140.9278,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2151128+675611 20260410.4278 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J223619.87+730041.5,2461140.9278,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J223619.87+730041.5 20260410.4278 11.11CV 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
ASASSN-V J215318.15+660450.3,2461140.9278,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215318.15+660450.3 20260410.4278 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
First image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Last image: 2461140.92812249 10.04.2026 10:16:19.783 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14491
Objects passed selection criteria: 14423
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 10933.8
Average stars matched: 9916 (90.6917 %)
Memory usage VmPeak: 117520 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 06:07:22 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
First image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Last image: 2461140.92812249 10.04.2026 10:16:19.783 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 150
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 36 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): 90025
Objects passed selection criteria: 89753
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 67973
Average stars matched: 61898.2 (91.063 %)
Memory usage VmPeak: 1868712 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 06:09:08 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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: 2461140.92755987
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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits exists and is non-empty
Saving wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits to local_wcs_cache/
'wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits' -> 'local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits'
wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits exists and is non-empty
Saving wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits to local_wcs_cache/
'wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits' -> 'local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:00.372 +70:00:00.06
Angular distance between the image centers 0.0254 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:00.275 +69:59:37.52
Angular distance between the image centers 0.0250 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:00.372 +70:00:00.06
Second-epoch second image center 21:36:00.275 +69:59:37.52
Angular distance between the image centers 0.00626 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits &> /tmp/tmp.Qe4GbK7Yyb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.MjEmQsH22p
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits &> /tmp/tmp.QrGHtDPAoX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits &> /tmp/tmp.lAb9JfGbxU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat' -> 'wcsmag.cat'
Read 14757 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 297.1683 to 352.6355 deg, Dec +62.8550 to +75.5006 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 297.1683 to 352.6355 deg, Dec 62.8550 to 75.5006 deg
Loaded 16171 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): 8237 out of 8864 total matches.
Matched with Tycho-2 8864 out of 14757 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917528
a=0.000000 b=1.000000 c=22.917528
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
2.4 pix Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
3.2 pix fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
3.2 pix fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Limiting magnitude estimates:
15.0 mag. Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
15.0 mag. Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
14.7 mag. fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
14.7 mag. fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (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.Qe4GbK7Yyb (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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1317, passed=14757
Got 14757 stars (including 13425 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 14757 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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.MjEmQsH22p (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/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1330, passed=14774
Got 14774 stars (including 13430 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 14774 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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.QrGHtDPAoX (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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1261, passed=12402
Got 12402 stars (including 11139 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 12402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 12078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 12078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 12078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits -region wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.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.lAb9JfGbxU (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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1302, passed=12413
Got 12413 stars (including 11107 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 12413 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits -region wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
Saving fully-calibrated image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits'
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits'
Preparing the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09617.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20658_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 20658_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:57:26.51 +65:20:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22270_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22270_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:08:26.24 +68:18:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22365_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22365_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:30:54.62 +73:29:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22405_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22405_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:49:41.83 +72:15:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22521_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22521_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:00:26.70 +67:59:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22552_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22552_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:53:32.21 +70:39:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.020 2271811994760308480 313.38407784841 +70.66625217830 11.6742 10.7994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22556_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22556_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:26:19.17 +69:38:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22624_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22624_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:57:31.57 +66:09:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22732_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22732_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:20:47.16 +68:08:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22762_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22762_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:12:13.77 +71:03:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22885_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22885_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:18:25.82 +67:05:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22911_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22911_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:54:53.91 +66:26:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.483 2245806620619017728 313.72477920144 +66.44470242743 12.3241 11.6207 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22991_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 22991_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:16:58.08 +70:15:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.804 2270861879275513856 319.24181495309 +70.26218670384 10.7636 9.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23035_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23035_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:55:34.38 +67:08:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23087_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23087_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:56:14.66 +66:19:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 4.883 2245801462359668096 314.05794731389 +66.32775408127 12.0387 11.1402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23122_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23122_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:06:54.65 +69:38:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.053 2270768004173225088 316.72850922986 +69.64536722353 12.0386 11.5835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23166_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23166_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:41:43.23 +67:40:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.865 2222836070368208256 325.43073865663 +67.68027429660 11.3742 10.2167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23222_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23222_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:52:46.48 +72:58:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.296 2272907658096830592 328.19426493907 +72.97697431485 10.9637 9.5193 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23387_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 23387_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:39:46.00 +65:56:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.726 2220987477787764480 324.94182248351 +65.94089416448 12.3654 11.9987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09617_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 09617_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09350_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 09350_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07957_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 07957_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06161_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 06161_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:26:54.26 +70:13:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09448_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 09448_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Cep-04-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 ####
22:02:02.39 +68:24:33.3
21:39:25.58 +67:58:24.9
21:44:42.04 +67:49:29.9
21:46:12.09 +67:38:12.9
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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits exists and is non-empty
wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits exists and is non-empty
wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:00.372 +70:00:00.06
Angular distance between the image centers 0.0254 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:00.275 +69:59:37.52
Angular distance between the image centers 0.0250 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:00.372 +70:00:00.06
Second-epoch second image center 21:36:00.275 +69:59:37.52
Angular distance between the image centers 0.00626 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits &> /tmp/tmp.OtRNrvdHdw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.WuxqS1ZdsC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits &> /tmp/tmp.QvaNXyn1vQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits &> /tmp/tmp.PtUyWbn02i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat' -> 'wcsmag.cat'
Read 98064 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 296.8277 to 352.6354 deg, Dec +62.7521 to +75.5202 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 296.8277 to 352.6354 deg, Dec 62.7521 to 75.5202 deg
Loaded 16494 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): 7206 out of 9231 total matches.
Matched with Tycho-2 9231 out of 98064 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.759782
a=0.000000 b=1.000000 c=22.759782
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 120 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
2.2 pix Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
2.9 pix fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
2.9 pix fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Limiting magnitude estimates:
15.2 mag. Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
15.2 mag. Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
14.8 mag. fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
14.8 mag. fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.1 (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.OtRNrvdHdw (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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=9697, passed=98031
Got 98031 stars (including 88176 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 98031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 763 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 96030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 763 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 96030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 96030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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.WuxqS1ZdsC (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/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=9846, passed=98099
Got 98099 stars (including 88083 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 98099 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 763 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 95822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 763 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 95822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 95821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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.QvaNXyn1vQ (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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=8770, passed=65513
Got 65513 stars (including 56692 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 65513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 63334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 63333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 63332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits -region wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.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.PtUyWbn02i (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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=8714, passed=65479
Got 65479 stars (including 56718 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 65479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 63746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 63746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 63745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits -region wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Saving fully-calibrated image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-15-31_20.00sec_-4.90C_LIGHT_0314.fits
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.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_2026-04-10_CI_Cep-04-Q2b1x1_052025_TTUQ2b1x1_855_gkhyQauz/wcs_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315.fits
Preparing the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out10712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out123720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out127862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out08218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95622.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 12s
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Considering the candidate 115482_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 115482_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:53:39.31 +73:23:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115490_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 115490_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:43:51.32 +69:58:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115491_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 115491_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 115497_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 115497_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:12:26.06 +68:13:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115498_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 115498_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:45:04.33 +69:04:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115499_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 115499_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 116996_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 116996_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 117433_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 117433_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:30:54.98 +73:29:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118016_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 118016_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:57:26.03 +67:09:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118147_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 118147_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:12:27.67 +73:19:24.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 119103_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 119103_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 119163_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 119163_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:06:39.61 +71:27:10.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 119256_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 119256_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 120117_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 120117_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:25:25.74 +70:27:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120139_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 120139_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:09:55.77 +65:56:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120664_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 120664_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:54:14.28 +66:18:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120670_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 120670_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:45:31.96 +72:11:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120783_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 120783_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:49:16.14 +71:47:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121085_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 121085_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:57:35.06 +66:07:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122956_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 122956_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:15:21.10 +66:32:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123164_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 123164_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:52:25.10 +68:46:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123269_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 123269_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:05:09.19 +71:21:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123284_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 123284_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:48:42.37 +68:15:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123720_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 123720_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:53:55.07 +67:40:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.269 2270123797735373056 313.47782337833 +67.68191332036 13.3779 12.4618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 123826_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 123826_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:40:29.57 +68:24:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124088_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124088_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:18:12.17 +65:43:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124155_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124155_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:27:54.38 +70:49:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124188_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124188_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:32:16.14 +72:50:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124563_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124563_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:30:47.88 +68:16:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124614_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124614_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:48:40.21 +68:15:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124703_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124703_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:25:22.14 +67:36:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124845_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 124845_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:25:21.44 +70:27:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125034_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125034_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:47:08.79 +69:54:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125194_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125194_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 125281_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125281_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:00:02.20 +72:43:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125291_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125291_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:52:51.71 +69:32:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125326_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125326_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:17:52.95 +66:38:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125410_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125410_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 125785_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125785_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:57:23.27 +70:27:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125865_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 125865_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:29:52.93 +73:20:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126383_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 126383_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:30:22.72 +70:19:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126481_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 126481_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:13:27.42 +66:29:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126545_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 126545_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:43:39.63 +68:38:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126783_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 126783_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:52:52.90 +69:03:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127330_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 127330_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:56:28.56 +67:47:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127827_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 127827_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 127862_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 127862_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:02:19.38 +68:37:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 5.078 2270291507618939904 315.58396704606 +68.61666072819 14.5893 13.8543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128158_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128158_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:57:03.30 +65:39:10.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
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Considering the candidate 128261_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128261_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:50:20.11 +68:12:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.955 2222958253598631040 327.58391967267 +68.20212572534 12.8803 11.4071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128263_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128263_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:54:06.88 +72:08:59.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 128544_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128544_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:29:27.39 +68:42:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.035 2222436359233094400 322.36266298683 +68.71377803505 12.7710 11.3073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128794_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128794_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:45:35.09 +66:18:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128805_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128805_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:15:04.98 +66:28:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.766 2221625851662980736 318.77080506557 +66.47114943560 13.1290 11.6615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128885_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128885_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:25:40.13 +68:47:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128943_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 128943_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:46:41.84 +72:22:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129237_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129237_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:37:21.42 +66:26:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.999 2221062764271092224 324.33961819774 +66.44674237371 13.0907 11.4971 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129484_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129484_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:24:08.42 +71:27:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.511 2229736227386654336 336.03768530262 +71.46323899436 13.3445 11.9498 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129558_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129558_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:18:15.86 +69:18:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 0.826 2270550820564185856 319.56549128252 +69.30210036065 14.4905 13.8527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129595_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129595_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:45:36.23 +71:10:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.147 2224601370644459904 326.40070210747 +71.18350737077 13.2933 11.8882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129634_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129634_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:45:20.33 +71:55:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 0.498 2274993431654632832 311.33487622540 +71.91701088865 14.4276 13.4843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129661_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129661_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:27:31.78 +71:48:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.234 2272599554322996224 321.88075265683 +71.81661748246 10.8784 9.5616 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129831_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129831_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:49:13.39 +71:53:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.824 2272787703954580736 327.30704616621 +71.89643459116 12.5835 10.9971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129854_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129854_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:59:23.20 +68:14:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 2.293 2270256357606156160 314.84531535145 +68.24546747123 14.3789 13.1014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129909_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 129909_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:47:23.33 +68:50:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129927_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 129927_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 130062_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130062_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:06:06.57 +69:13:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130074_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130074_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:47:47.55 +71:11:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.837 2274891211432784128 311.94744819992 +71.19427472597 14.3729 13.4691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130132_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130132_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:08:48.36 +70:21:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 0.524 2270902045809494528 317.20113839967 +70.36278112915 14.2790 13.3119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130151_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130151_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:16:56.41 +68:40:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.396 2270426266512567680 319.23537884178 +68.68171534644 14.1547 13.0233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130187_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130187_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 130284_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130284_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:03:06.87 +68:02:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.359 2270053394631120384 315.77774941688 +68.04870103062 14.6298 13.6998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130345_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130345_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:19:57.77 +72:09:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.347 2273358835820991872 319.99157578512 +72.15815213966 14.0532 12.9050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130379_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130379_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:23:41.28 +71:08:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.254 2272415317406455680 320.92221637125 +71.14190683846 14.4581 13.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130389_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130389_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:13:34.19 +69:59:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 0.867 2270829546761419520 318.39212261139 +69.99698282790 14.5194 13.9280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130409_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130409_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:13:07.22 +69:55:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.527 2270827519536857984 318.28028488041 +69.91754554883 14.2228 13.1118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130453_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130453_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:25:22.81 +71:07:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.699 2272413015304009216 321.34494957287 +71.12533088327 14.5257 13.5472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130460_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130460_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:08:19.35 +71:53:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 5.141 2230510936406516736 332.08491464873 +71.88462116305 13.4290 11.9802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130471_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130471_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:23:58.81 +67:28:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.497 2222076376552575744 320.99440655347 +67.46980164550 13.1441 11.5238 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 130602_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 130602_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:27:10.68 +71:14:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94801_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 94801_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:40:08.80 +68:02:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22171_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 22171_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 83794_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 83794_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:56:13.41 +66:17:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84706_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 84706_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 90959_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 90959_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 108678_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 108678_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:02:07.60 +73:25:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108119_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 108119_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:49:51.27 +68:31:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93404_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 93404_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 63973_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 63973_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:07:35.57 +67:10:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90501_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 90501_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 72037_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 72037_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 50985_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 50985_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 38268_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 38268_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:24:58.56 +69:20:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53059_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 53059_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:02:02.40 +68:24:33.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 19165_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 19165_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 92392_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 92392_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:46:12.08 +67:38:12.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 87156_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 87156_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:54:36.29 +66:45:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50462_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 50462_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:23:07.53 +68:07:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28272_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 28272_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:11:50.11 +70:56:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15352_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 15352_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 81845_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 81845_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 17211_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 17211_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 10813_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 10813_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 93771_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 93771_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:44:42.03 +67:49:30.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53023_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 53023_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:08:26.23 +68:18:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92196_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 92196_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 94155_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 94155_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:39:25.57 +67:58:25.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 25099_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 25099_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 20:49:41.88 +72:15:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83711_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 83711_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 84418_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 84418_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 40731_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 40731_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:26:54.25 +70:13:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83925_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 83925_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:41:16.51 +66:40:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67965_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 67965_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 64661_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 64661_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:18:25.80 +67:05:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40523_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 40523_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 109789_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 109789_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:55:24.66 +69:11:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95622_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 95622_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 08218_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 08218_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 81859_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
Preparing report for the candidate 81859_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
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Considering the candidate 90213_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 90213_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 21:55:34.35 +67:08:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10712_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315
The candidate 10712_fd_Cep-04-Q2b1x1_2026-04-10_05-16-19_20.00sec_-4.90C_LIGHT_0315 did not pass the final checks
**** FOUND 22:08:13.75 +73:26:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.595 2278891402236539904 332.05986611329 +73.45090576037 12.4510 10.9801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 43s
Prepared the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:02:02.39 +68:24:33.3
21:39:25.58 +67:58:24.9
21:44:42.04 +67:49:29.9
21:46:12.09 +67:38:12.9
22:36:18.73 +73:00:38.5
22:05:47.89 +73:28:58.4
22:06:59.30 +66:57:59.7
22:13:38.25 +65:49:26.8
21:04:40.52 +70:34:12.4
20:56:12.83 +73:33:31.2
21:47:44.83 +72:57:44.5
22:19:51.31 +72:01:23.3
21:54:53.04 +72:10:39.3
21:13:19.08 +70:24:05.0
22:23:32.30 +68:04:35.8
21:33:19.66 +65:43:27.6
21:04:15.98 +67:42:47.1
21:58:22.01 +65:57:04.7
21:53:17.89 +66:04:53.3
21:47:36.60 +66:28:36.8
22:02:27.09 +66:12:49.7
21:44:03.69 +66:39:14.0
22:21:27.40 +66:26:46.7
21:52:21.61 +67:18:10.6
22:17:44.36 +66:46:16.6
22:16:44.67 +66:59:41.9
21:51:12.82 +67:56:13.4
########### Completed Cep-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:46:12.09 +67:38:12.9
21:39:25.58 +67:58:24.9
22:02:02.39 +68:24:33.3
21:44:42.04 +67:49:29.9
22:06:59.30 +66:57:59.7
22:13:38.25 +65:49:26.8
21:04:40.52 +70:34:12.4
21:54:53.04 +72:10:39.3
21:44:03.69 +66:39:14.0
21:52:21.61 +67:18:10.6
22:16:44.67 +66:59:41.9
22:21:27.40 +66:26:46.7
21:04:15.98 +67:42:47.1
22:23:32.30 +68:04:35.8
22:19:51.31 +72:01:23.3
20:56:12.83 +73:33:31.2
21:58:22.01 +65:57:04.7
21:47:44.83 +72:57:44.5
22:05:47.89 +73:28:58.4
22:17:44.36 +66:46:16.6
21:47:36.60 +66:28:36.8
22:02:27.09 +66:12:49.7
21:33:19.66 +65:43:27.6
21:13:19.08 +70:24:05.0
21:51:12.82 +67:56:13.4
22:36:18.73 +73:00:38.5
21:53:17.89 +66:04:53.3
###################################################################################
21:46:12.09 +67:38:12.9 -- not an asteroid (will add it to exclusion list)
21:39:25.58 +67:58:24.9 -- not an asteroid (will add it to exclusion list)
22:02:02.39 +68:24:33.3 -- not an asteroid (will add it to exclusion list)
21:44:42.04 +67:49:29.9 -- not an asteroid (will add it to exclusion list)
22:06:59.30 +66:57:59.7 -- not an asteroid (will add it to exclusion list)
22:13:38.25 +65:49:26.8 -- not an asteroid (will add it to exclusion list)
21:04:40.52 +70:34:12.4 -- not an asteroid (will add it to exclusion list)
21:54:53.04 +72:10:39.3 -- not an asteroid (will add it to exclusion list)
21:44:03.69 +66:39:14.0 -- not an asteroid (will add it to exclusion list)
21:52:21.61 +67:18:10.6 -- not an asteroid (will add it to exclusion list)
22:16:44.67 +66:59:41.9 -- not an asteroid (will add it to exclusion list)
22:21:27.40 +66:26:46.7 -- not an asteroid (will add it to exclusion list)
21:04:15.98 +67:42:47.1 -- not an asteroid (will add it to exclusion list)
22:23:32.30 +68:04:35.8 -- not an asteroid (will add it to exclusion list)
22:19:51.31 +72:01:23.3 -- not an asteroid (will add it to exclusion list)
20:56:12.83 +73:33:31.2 -- not an asteroid (will add it to exclusion list)
21:58:22.01 +65:57:04.7 -- not an asteroid (will add it to exclusion list)
21:47:44.83 +72:57:44.5 -- not an asteroid (will add it to exclusion list)
22:05:47.89 +73:28:58.4 -- not an asteroid (will add it to exclusion list)
22:17:44.36 +66:46:16.6 -- not an asteroid (will add it to exclusion list)
21:47:36.60 +66:28:36.8 -- not an asteroid (will add it to exclusion list)
22:02:27.09 +66:12:49.7 -- not an asteroid (will add it to exclusion list)
21:33:19.66 +65:43:27.6 -- not an asteroid (will add it to exclusion list)
21:13:19.08 +70:24:05.0 -- not an asteroid (will add it to exclusion list)
21:51:12.82 +67:56:13.4 -- not an asteroid (will add it to exclusion list)
22:36:18.73 +73:00:38.5 -- not an asteroid (will add it to exclusion list)
21:53:17.89 +66:04:53.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:56:12.83 +73:33:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:15.98 +67:42:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:40.52 +70:34:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:19.08 +70:24:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:19.66 +65:43:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:25.58 +67:58:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.69 +66:39:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:42.04 +67:49:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:12.09 +67:38:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:36.60 +66:28:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:44.83 +72:57:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:12.82 +67:56:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:21.61 +67:18:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.89 +66:04:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:53.04 +72:10:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:22.01 +65:57:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:02.39 +68:24:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.09 +66:12:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:47.89 +73:28:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:59.30 +66:57:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:38.25 +65:49:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:44.67 +66:59:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:44.36 +66:46:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:51.31 +72:01:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:27.40 +66:26:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:32.30 +68:04:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:36:18.73 +73:00:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:56:12.83 +73:33:31.2 -- a known variable star
21:04:15.98 +67:42:47.1 -- a known variable star
21:04:40.52 +70:34:12.4 -- not a known variable star
21:13:19.08 +70:24:05.0 -- a known variable star
21:33:19.66 +65:43:27.6 -- a known variable star
21:39:25.58 +67:58:24.9 -- a known variable star
21:44:03.69 +66:39:14.0 -- a known variable star
21:44:42.04 +67:49:29.9 -- a known variable star
21:46:12.09 +67:38:12.9 -- a known variable star
21:47:36.60 +66:28:36.8 -- a known variable star
21:47:44.83 +72:57:44.5 -- a known variable star
21:51:12.82 +67:56:13.4 -- a known variable star
21:52:21.61 +67:18:10.6 -- a known variable star
21:53:17.89 +66:04:53.3 -- a known variable star
21:54:53.04 +72:10:39.3 -- a known variable star
21:58:22.01 +65:57:04.7 -- a known variable star
22:02:02.39 +68:24:33.3 -- a known variable star
22:02:27.09 +66:12:49.7 -- a known variable star
22:05:47.89 +73:28:58.4 -- a known variable star
22:06:59.30 +66:57:59.7 -- a known variable star
22:13:38.25 +65:49:26.8 -- not a known variable star
22:16:44.67 +66:59:41.9 -- a known variable star
22:17:44.36 +66:46:16.6 -- a known variable star
22:19:51.31 +72:01:23.3 -- a known variable star
22:21:27.40 +66:26:46.7 -- a known variable star
22:23:32.30 +68:04:35.8 -- a known variable star
22:36:18.73 +73:00:38.5 -- a known variable star
Found 2 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
27 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 ####
20:56:12.83 +73:33:31.2
21:04:15.98 +67:42:47.1
21:04:40.52 +70:34:12.4
21:13:19.08 +70:24:05.0
21:33:19.66 +65:43:27.6
21:39:25.58 +67:58:24.9
21:44:03.69 +66:39:14.0
21:44:42.04 +67:49:29.9
21:46:12.09 +67:38:12.9
21:47:36.60 +66:28:36.8
21:47:44.83 +72:57:44.5
21:51:12.82 +67:56:13.4
21:52:21.61 +67:18:10.6
21:53:17.89 +66:04:53.3
21:54:53.04 +72:10:39.3
21:58:22.01 +65:57:04.7
22:02:02.39 +68:24:33.3
22:02:27.09 +66:12:49.7
22:05:47.89 +73:28:58.4
22:06:59.30 +66:57:59.7
22:13:38.25 +65:49:26.8
22:16:44.67 +66:59:41.9
22:17:44.36 +66:46:16.6
22:19:51.31 +72:01:23.3
22:21:27.40 +66:26:46.7
22:23:32.30 +68:04:35.8
22:36:18.73 +73:00:38.5
20:53:32.21 +70:39:57.5
20:54:53.91 +66:26:40.5
21:16:58.08 +70:15:43.1
20:56:14.66 +66:19:38.1
21:06:54.65 +69:38:43.0
21:41:43.23 +67:40:49.2
21:52:46.48 +72:58:34.9
21:39:46.00 +65:56:23.5
22:08:13.75 +73:26:59.5
20:53:55.07 +67:40:54.5
21:02:19.38 +68:37:02.8
20:57:03.30 +65:39:10.3
21:50:20.11 +68:12:09.6
20:54:06.88 +72:08:59.3
21:29:27.39 +68:42:50.3
21:15:04.98 +66:28:16.9
21:37:21.42 +66:26:50.2
22:24:08.42 +71:27:45.8
21:18:15.86 +69:18:07.9
21:45:36.23 +71:10:58.5
20:45:20.33 +71:55:01.7
21:27:31.78 +71:48:58.6
21:49:13.39 +71:53:46.0
20:59:23.20 +68:14:45.1
20:47:47.55 +71:11:39.1
21:08:48.36 +70:21:46.3
21:16:56.41 +68:40:55.5
21:03:06.87 +68:02:56.0
21:19:57.77 +72:09:28.4
21:23:41.28 +71:08:30.9
21:13:34.19 +69:59:49.9
21:13:07.22 +69:55:02.7
21:25:22.81 +71:07:30.5
22:08:19.35 +71:53:02.8
21:23:58.81 +67:28:12.5
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461140.92755987 -observatory V36
23:39:22.18 -04:48:36.9 Mercury (0.2mag)
02:41:39.84 +15:39:28.4 Venus (-3.9mag)
00:01:59.75 -00:52:51.3 Mars (1.2mag)
07:10:15.95 +22:50:01.2 Jupiter (-2.1mag)
00:26:40.93 +00:33:19.8 Saturn (0.9mag)
03:46:33.11 +19:43:47.1 Uranus (5.8mag)
00:10:06.15 -00:20:02.2 Neptune (7.8mag)
20:33:28.95 -22:52:27.1 Pluto (14.5mag)
19:43:11.15 -25:48:12.8 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 362 Apr 10 06:07 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.92755987:
07:10:08.60 +22:50:16.8 Io (5.7mag)
07:10:18.81 +22:49:52.2 Europa (5.9mag)
07:10:10.26 +22:50:05.4 Ganymede (5.3mag)
07:09:57.13 +22:50:46.5 Callisto (6.6mag)
07:13:49.97 +22:40:20.4 Himalia (15.3mag)
07:10:19.57 +22:49:54.9 Thebe (16.2mag)
07:13:53.80 +23:09:54.6 Elara (17.3mag)
07:08:46.09 +23:32:56.4 Pasiphae (17.4mag)
07:18:42.81 +22:47:27.4 Carme (18.5mag)
00:26:51.41 +00:33:11.4 Titan (8.8mag)
00:26:38.57 +00:33:35.5 Rhea (10.1mag)
00:26:31.92 +00:34:20.6 Iapetus (11.5mag)
00:26:54.86 +00:33:09.3 Hyperion (14.8mag)
00:28:22.11 +00:42:43.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 10 06:07 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.92755987:
15:10:12.57 -12:02:50.1 JWST
20:21:28.37 -06:54:36.3 Chandra
08:55:06.94 -50:34:58.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 10 06:07 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.92755987 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:27.24 -28:27:45.1 13.9mag P/2010 H2 (Vales)
05:02:51.20 -69:55:56.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:18.94 +31:24:03.6 17.2mag C/2017 K2 (PANSTARRS)
17:30:50.59 +09:52:56.6 17.6mag C/2021 G2 (ATLAS)
23:08:39.68 +29:00:58.6 17.0mag C/2022 E2 (ATLAS)
04:22:47.94 +25:53:04.2 15.9mag C/2022 N2 (PANSTARRS)
09:02:23.43 +31:58:06.8 16.2mag C/2022 QE78 (ATLAS)
08:30:20.66 -00:45:21.0 17.3mag C/2022 R6 (PANSTARRS)
18:54:54.60 +18:03:36.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:22.63 -11:36:07.7 17.5mag P/2023 B1 (PANSTARRS)
09:10:24.87 -12:47:27.8 17.6mag C/2023 F3 (ATLAS)
21:48:20.96 +62:35:31.2 17.5mag C/2023 H5 (Lemmon)
19:23:37.23 -03:39:10.6 14.2mag C/2023 R1 (PANSTARRS)
21:40:22.77 +85:09:19.6 17.8mag C/2023 X2 (Lemmon)
06:15:39.71 +63:32:44.9 17.1mag C/2024 A1 (ATLAS)
05:00:59.12 +16:18:38.8 10.7mag C/2024 E1 (Wierzchos)
16:22:42.90 +05:28:29.6 17.4mag C/2024 G6 (ATLAS)
20:19:05.49 +13:46:58.8 14.7mag C/2024 J3 (ATLAS)
03:21:25.57 -23:14:50.1 16.4mag C/2024 T5 (ATLAS)
05:12:04.57 +46:42:22.8 17.7mag C/2025 J1 (Borisov)
14:01:57.15 +41:20:01.6 14.9mag C/2025 L1 (ATLAS)
03:16:39.12 -25:21:47.5 17.8mag C/2025 Q3 (ATLAS)
23:07:50.57 +19:41:30.3 9.4mag C/2025 R3 (PANSTARRS)
12:56:32.53 +02:39:58.3 17.5mag C/2025 Y1 (ATLAS)
02:33:04.82 +03:26:57.8 11.1mag C/2026 A1 (MAPS)
23:43:29.41 +36:08:37.4 14.4mag C/2026 B2 (Sun-Gao)
18:32:04.14 -10:00:40.2 12.2mag 10P/Tempel
15:07:40.54 +03:45:11.4 13.5mag 24P/Schaumasse
11:04:23.91 -01:42:45.7 15.7mag 29P/Schwassmann-Wachmann
17:58:56.03 -09:49:22.2 17.8mag 40P/Vaisala
10:38:04.07 -04:33:48.9 16.8mag 43P/Wolf-Harrington
01:40:04.03 +16:31:54.8 17.2mag 47P/Ashbrook-Jackson
07:00:40.33 +38:11:50.2 17.0mag 63P/Wild
23:21:52.81 -12:07:41.8 15.7mag 65P/Gunn
03:48:33.17 +19:17:42.1 15.9mag 76P/West-Kohoutek-Ikemura
00:53:18.79 +07:07:42.3 14.4mag 78P/Gehrels
22:45:54.39 -11:02:06.7 14.6mag 88P/Howell
01:54:47.43 +19:07:54.5 15.1mag 93P/Lovas
04:44:28.86 +31:58:44.2 16.3mag 123P/West-Hartley
08:22:07.20 +40:55:59.5 16.2mag 124P/Mrkos
02:24:39.12 +13:44:33.3 16.4mag 128P/Shoemaker-Holt
02:36:38.20 +13:48:01.3 17.5mag 131P/Mueller
00:57:14.77 +11:14:04.7 10.9mag 141P/Machholz
01:06:51.64 +02:46:48.0 11.0mag 141P-A/Machholz
23:55:00.79 -01:04:21.1 13.5mag 141P-D/Machholz
01:36:36.33 +04:30:12.6 17.9mag 141P-I/Machholz
00:46:52.60 -04:19:06.2 15.2mag 162P/SidingSpring
10:29:47.50 +31:14:03.4 17.9mag 164P/Christensen
06:26:12.58 +24:24:51.3 17.9mag 198P/ODAS
15:01:18.92 -00:40:47.2 17.5mag 210P/Christensen
21:22:16.02 -12:47:47.6 17.5mag 218P/LINEAR
17:14:42.59 -14:35:34.2 16.2mag 235P/LINEAR
05:22:33.06 +34:14:46.8 16.7mag 240P/NEAT
07:35:54.59 -05:47:16.7 17.7mag 242P/Spahr
15:44:39.57 +06:36:43.0 17.5mag 391P/Kowalski
07:32:12.00 +21:20:29.2 17.6mag 450P/LONEOS
05:27:50.66 +45:21:34.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 10 06:07 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 10 06:07 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 10 06:07 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:34:23.750 +44:37:52.78 AT 2026ilj 2026-03-28.82 20.88
10:22:27.680 +34:19:20.03 AT 2026ili 2026-03-26.73 20.17
11:13:24.630 +35:18:50.10 AT 2026ilh 2026-03-26.72 20.38
11:08:00.250 +43:03:49.46 AT 2026ilg 2026-03-26.71 20.44
12:43:47.830 +50:53:50.11 AT 2026ilf 2026-03-24.69 20.5
11:22:31.710 +50:15:03.24 AT 2026ile 2026-03-24.66 21.56
11:51:00.240 +50:24:44.16 AT 2026ild 2026-03-24.66 22.08
16:09:39.700 +41:58:22.06 AT 2026ilc 2026-03-23.81 21.36
12:43:38.630 +34:06:30.25 AT 2026ilb 2026-03-22.71 21.66
13:18:04.360 +55:35:55.40 AT 2026ila 2026-03-19.80 21.3
10:59:06.280 +46:45:22.92 AT 2026ikz 2026-03-19.66 21.07
13:16:17.130 +52:30:17.46 AT 2026iky 2026-03-19.80 20.85
10:24:12.482 +42:11:55.90 AT 2026ikx 2026-03-07.58 21.39
10:41:54.510 -01:26:19.22 AT 2026ikw 2026-04-03.66 20.82
10:43:38.720 +04:39:38.40 AT 2026ikv 2026-03-22.64 22.16
10:34:06.300 +04:06:25.11 AT 2026iku 2026-03-19.63 22.6
11:40:08.790 +04:58:19.09 AT 2026ikt 2026-03-22.66 22.08
11:22:52.580 +02:15:24.51 AT 2026iks 2026-03-15.61 21.97
10:28:53.530 +01:08:32.24 AT 2026ikr 2026-03-15.59 22.4
11:00:12.130 -00:25:26.16 AT 2026ikq 2026-03-13.74 21.8
-rw-r--r-- 1 apache apache 30K Apr 10 06:07 tns_transients_list.txt
