This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop
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!
TCP 2026 04 02.3969* 00 54 34.61 +72 29 30.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 04304-00387,2461132.8969,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04304-00387 20260402.3969 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 01 01 56.80 +69 39 31.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532979293672722048,2461132.8969,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 532979293672722048 20260402.3969 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 54 22.20 +68 40 52.6 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0054236+684060,2461132.8969,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0054236+684060 20260402.3969 12.79CV 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!
TCP 2026 04 02.3969* 00 57 50.51 +68 13 41.2 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0057522+681341,2461132.8969,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0057522+681341 20260402.3969 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 55 32.73 +68 28 54.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0880 Cas,2461132.8969,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0880 Cas 20260402.3969 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 01 03 55.88 +70 33 17.8 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0103557+703317,2461132.8969,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0103557+703317 20260402.3969 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 01 02 42.21 +68 37 31.0 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010243.37+683730.9,2461132.8969,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J010243.37+683730.9 20260402.3969 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 15 07.58 +66 20 41.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8969,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260402.3969 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 55 27.97 +70 00 52.5 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1266 Cas,2461132.8969,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1266 Cas 20260402.3969 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 30 24.02 +69 47 38.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1257 Cas,2461132.8969,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1257 Cas 20260402.3969 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 47 59.72 +72 47 49.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0048021+724805,2461132.8969,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0048021+724805 20260402.3969 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2337044+684351,2461132.8969,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2337044+684351 20260402.3969 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 45 50.08 +69 33 37.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0045524+693336,2461132.8969,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0045524+693336 20260402.3969 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2300118+700223,2461132.8969,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2300118+700223 20260402.3969 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 37 27.36 +65 50 16.8 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003727.81+655013.4,2461132.8969,12.38,0.05,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
ASASSN-V J003727.81+655013.4 20260402.3969 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!
TCP 2026 04 02.3969* 00 19 04.13 +66 22 15.2 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1616511,2461132.8969,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1616511 20260402.3969 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 34 42.39 +65 40 12.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1626030,2461132.8969,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1626030 20260402.3969 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 31 25.25 +67 38 21.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1622640,2461132.8969,12.86,0.05,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 1622640 20260402.3969 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!
TCP 2026 04 02.3969* 00 38 54.20 +69 51 36.1 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 04299-01952,2461132.8969,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04299-01952 20260402.3969 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234757.29+683542.7,2461132.8969,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234757.29+683542.7 20260402.3969 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0005230+700948,2461132.8969,12.29,0.05,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 J0005230+700948 20260402.3969 12.29CV 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!
TCP 2026 04 02.3969* 00 34 08.57 +66 02 57.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 04027-00040,2461132.8969,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04027-00040 20260402.3969 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 01 00 04.55 +67 37 23.1 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1269 Cas,2461132.8969,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1269 Cas 20260402.3969 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 01 07 39.55 +70 34 55.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0107403+703455,2461132.8969,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0107403+703455 20260402.3969 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2320370+673213,2461132.8969,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2320370+673213 20260402.3969 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 201239,2461132.8969,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 201239 20260402.3969 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 39 22.29 +72 34 14.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0039234+723417,2461132.8969,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0039234+723417 20260402.3969 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 59 51.35 +70 29 37.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 533089111697804288,2461132.8969,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 533089111697804288 20260402.3969 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0015566+694231,2461132.8969,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0015566+694231 20260402.3969 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 46 37.08 +68 00 53.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 223609,2461132.8969,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 223609 20260402.3969 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 42 37.80 +67 20 06.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1199,2461132.8969,12.11,0.05,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
Mis V1199 20260402.3969 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235831.13+682317.6,2461132.8969,12.38,0.05,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
ASASSN-V J235831.13+682317.6 20260402.3969 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!
TCP 2026 04 02.3969* 00 40 46.36 +66 59 00.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0040470+665857,2461132.8969,11.55,0.05,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
NSVS J0040470+665857 20260402.3969 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J001029.53+670231.2,2461132.8969,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J001029.53+670231.2 20260402.3969 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 53 50.16 +70 20 05.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0053507+702007,2461132.8969,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0053507+702007 20260402.3969 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0025483+670931,2461132.8969,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0025483+670931 20260402.3969 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 59 30.96 +71 21 48.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 339575,2461132.8969,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 339575 20260402.3969 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 38 56.09 +68 02 34.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003856.59+680232.9,2461132.8969,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003856.59+680232.9 20260402.3969 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 30 26.02 +68 42 59.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1039 Cas,2461132.8969,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1039 Cas 20260402.3969 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 54 15.71 +68 03 44.1 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J005416.56+680344.7,2461132.8969,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J005416.56+680344.7 20260402.3969 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 33 33.14 +68 57 42.2 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003333.50+685742.2,2461132.8969,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003333.50+685742.2 20260402.3969 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3969* 00 50 34.62 +69 04 02.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 224448,2461132.8969,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 224448 20260402.3969 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234851.21+682436.5,2461132.8969,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234851.21+682436.5 20260402.3969 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461132.89725950 02.04.2026 09:31:53.221 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
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: 3 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): 14314
Objects passed selection criteria: 14210
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 9479.25
Average stars matched: 8953.75 (94.4563 %)
Memory usage VmPeak: 119072 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:35:12 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: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461132.89725950 02.04.2026 09:31:53.221 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 119
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: 18 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): 94752
Objects passed selection criteria: 94529
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 65383
Average stars matched: 61197.5 (93.5985 %)
Memory usage VmPeak: 1927512 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:36:49 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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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: 2461132.89658183
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits'
wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:57.371 +70:02:23.58
Angular distance between the image centers 0.04 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 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:55.900 +70:01:41.81
Angular distance between the image centers 0.03 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 23:59:57.371 +70:02:23.58
Second-epoch second image center 23:59:55.900 +70:01:41.81
Angular distance between the image centers 0.01179 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.YaNUyTE7hf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.6ES2tfh0kW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.qjAtUWqIoq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.NAlzS8TZnT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat' -> 'wcsmag.cat'
Read 16658 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0025 to 359.9970 deg, Dec +62.8658 to +75.5048 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 0.0025 to 359.9970 deg, Dec 62.8658 to 75.5048 deg
Loaded 84082 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): 8746 out of 9568 total matches.
Matched with Tycho-2 9568 out of 16658 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942221
a=0.000000 b=1.000000 c=22.942221
From vast_summary.log: estimated ref. image limiting mag.: -7.91
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 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
3.0 pix fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
3.0 pix fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Limiting magnitude estimates:
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
13.6 mag. fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
13.6 mag. fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.0 (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.YaNUyTE7hf (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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1610, passed=16658
Got 16658 stars (including 15034 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 16658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.9470 through 0 to 28.4123, gap 28.4123 to 332.9470
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
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...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.9477 through 0 to 28.4145, gap 28.4145 to 332.9477
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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.6ES2tfh0kW (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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1667, passed=16773
Got 16773 stars (including 15086 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 16773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 333.1738 through 0 to 27.8274, gap 27.8274 to 333.1738
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 338 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.96"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 333.1326 through 0 to 27.8046, gap 27.8046 to 333.1326
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 7.13"
Estimated accuracy of the plate solution: 5.47"
Excluding outliers - 386 stars left (next iteration limit 309)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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.qjAtUWqIoq (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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=479, passed=5646
Got 5646 stars (including 5163 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 5646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
RA wraps around 0/360 boundary: field RA 331.9634 through 0 to 27.8477, gap 27.8477 to 331.9634
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 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...
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 331.9633 through 0 to 27.8521, gap 27.8521 to 331.9633
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 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
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 0.95"
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-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.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.NAlzS8TZnT (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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=475, passed=5664
Got 5664 stars (including 5182 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 5664 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
RA wraps around 0/360 boundary: field RA 331.9635 through 0 to 27.8397, gap 27.8397 to 331.9635
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...
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 331.9633 through 0 to 27.8430, gap 27.8430 to 331.9633
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
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 972 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-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits'
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02818.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21227_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 21227_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:13:10.26 +73:51:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21435_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 21435_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 22:58:41.06 +69:50:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 1.504 2225778569644146560 344.67222181084 +69.84035670728 10.7212 10.4339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02818_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 02818_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Cep-03-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 ####
00:54:34.61 +72:29:30.2
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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:57.371 +70:02:23.58
Angular distance between the image centers 0.04 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 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:55.900 +70:01:41.81
Angular distance between the image centers 0.03 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 23:59:57.371 +70:02:23.58
Second-epoch second image center 23:59:55.900 +70:01:41.81
Angular distance between the image centers 0.01179 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.ZngVneDs4s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.q6T7HA0R6P
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.UgRiBA2asf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.7B3WcTNg5P
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat' -> 'wcsmag.cat'
Read 114234 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9997 deg, Dec +62.7863 to +75.5048 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 0.0012 to 359.9997 deg, Dec 62.7863 to 75.5048 deg
Loaded 84921 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): 7448 out of 9832 total matches.
Matched with Tycho-2 9832 out of 114234 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779293
a=0.000000 b=1.000000 c=22.779293
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.7 pix fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
2.7 pix fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Limiting magnitude estimates:
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
13.8 mag. fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
13.8 mag. fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZngVneDs4s (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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=12405, passed=114192
Got 114192 stars (including 101585 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 114192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.6411 through 0 to 28.4717, gap 28.4717 to 332.6411
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.8 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...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.6416 through 0 to 28.4739, gap 28.4739 to 332.6416
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.8 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
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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.q6T7HA0R6P (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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=12319, passed=113226
Got 113226 stars (including 100709 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 113226 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.7589 through 0 to 27.9073, gap 27.9073 to 332.7589
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 349 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.18"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.7145 through 0 to 27.8794, gap 27.8794 to 332.7145
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 414 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.74"
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 384 stars left (next iteration limit 322)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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.UgRiBA2asf (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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2246, passed=36441
Got 36441 stars (including 34141 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 36441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
RA wraps around 0/360 boundary: field RA 331.5955 through 0 to 27.8492, gap 27.8492 to 331.5955
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 331.5960 through 0 to 27.8507, gap 27.8507 to 331.5960
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.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.7B3WcTNg5P (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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2213, passed=36476
Got 36476 stars (including 34218 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 36476 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
RA wraps around 0/360 boundary: field RA 331.5940 through 0 to 27.8426, gap 27.8426 to 331.5940
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.5 to 75.3)
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...
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 331.5946 through 0 to 27.8442, gap 27.8442 to 331.5946
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.5 to 75.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 973 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_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-30-54_20.00sec_-15.00C_LIGHT_0051.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.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_2026-04-02_CI_Cep-03-Q2b1x1_043252_TTUQ2b1x1_17572_f4YjMVop/wcs_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052.fits
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out124978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95564.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 19s
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Considering the candidate 133077_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133077_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:40:57.13 +70:23:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.367 2215319980681429504 355.23855531800 +70.39592160064 13.1343 12.0908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133080_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133080_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:40:31.99 +70:27:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133082_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133082_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 22:52:39.97 +71:11:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.275 2226896807328841088 343.16544428725 +71.19688049966 13.1966 12.6431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133083_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133083_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 01:15:59.93 +71:37:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.401 534887191165999488 018.99819375223 +71.63123550238 12.3553 11.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133086_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133086_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:27:08.69 +69:16:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.624 2214819015695826816 351.78590612243 +69.27875248515 12.9428 12.3551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133088_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 133088_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
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Considering the candidate 133089_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133089_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 22:55:25.35 +70:54:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133090_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133090_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:08:58.01 +73:15:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.100 2231599865237235712 347.24170548174 +73.25613888564 11.3950 10.0844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133092_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133092_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 01:20:53.34 +72:50:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 4.616 535064109458063232 020.21790389528 +72.84205630208 11.3242 10.7878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133093_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133093_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:02:50.56 +70:18:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 3.337 2225824573034710016 345.71098026853 +70.30558750426 12.2522 11.6091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133095_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 133095_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:11:30.98 +67:30:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135034_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 135034_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:00:42.49 +71:53:22.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)
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Considering the candidate 135236_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 135236_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:25:09.22 +70:08:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.267 530907955501387264 006.29180217448 +70.14770473446 10.6987 9.5079 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135683_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 135683_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:48:13.00 +67:47:50.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136289_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136289_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 01:18:28.13 +72:54:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136389_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136389_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:18:16.45 +68:07:15.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136391_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136391_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:04:07.98 +70:48:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136426_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136426_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:25:32.53 +71:49:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136607_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136607_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:21:27.14 +67:49:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136674_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136674_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:04:59.63 +68:25:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.026 2213418164863072768 346.24623799680 +68.42581141600 12.5823 11.9217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 136938_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 136938_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:20:00.31 +73:55:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137016_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137016_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:05:14.57 +67:48:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137288_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137288_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:01:40.10 +73:38:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137337_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137337_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:57:59.51 +73:32:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.889 2228134990562620160 359.49738074360 +73.54101836338 12.3324 11.3309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137390_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137390_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:49:46.25 +68:33:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.638 2211203855822692096 357.44226413935 +68.55010279362 11.9455 10.0524 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137610_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137610_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:36:41.33 +67:50:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137617_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137617_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:07:10.86 +67:17:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137685_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137685_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:27:09.43 +65:38:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137730_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137730_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:45:13.36 +71:37:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.295 536581362485909120 011.30739433220 +71.62575503559 11.4103 9.8788 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137750_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137750_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:05:33.99 +69:17:10.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137854_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137854_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:37:58.00 +72:54:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137866_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 137866_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:27:23.04 +70:17:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138008_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138008_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:20:50.34 +69:24:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.490 530497459710957696 005.21171681320 +69.41272750669 11.4944 9.9037 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138203_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138203_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:01:01.16 +70:56:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138236_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138236_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 22:52:34.42 +67:58:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138333_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 138333_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138371_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138371_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:44:08.61 +70:18:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138397_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138397_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:55:48.21 +72:48:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138486_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138486_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:04:29.45 +68:13:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.074 2213201702810474368 346.12159439399 +68.22773483521 13.1332 12.4085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138488_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138488_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 22:55:55.87 +68:14:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.476 2213350858435303424 343.98215581979 +68.23296490851 13.0915 12.4694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138550_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138550_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:37:18.63 +68:45:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138700_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138700_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:20:24.83 +69:47:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.456 530885449876232320 005.10617167529 +69.79915297819 11.1978 9.5813 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138718_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138718_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:39:03.62 +74:02:20.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138749_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138749_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:22:15.80 +71:28:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138758_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 138758_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138780_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138780_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:39:31.19 +70:47:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138974_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 138974_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:02:13.63 +70:13:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139013_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139013_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:12:43.99 +67:24:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139069_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139069_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:33:05.40 +71:00:03.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139141_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139141_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:28:56.54 +72:14:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139259_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139259_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:18:56.43 +71:20:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.471 2227476280017886080 349.73443208262 +71.33848202901 12.7227 11.6205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139279_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139279_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:57:25.86 +72:50:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139397_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139397_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:14:27.73 +70:35:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139617_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139617_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:05:57.13 +69:37:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.628 2225548806073889536 346.48514878066 +69.62317435646 11.6012 9.8580 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139630_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139630_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:06:23.91 +70:05:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139645_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 139645_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:03:52.46 +71:11:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124978_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 124978_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:23:46.90 +70:56:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.453 531064395393799936 005.94452375057 +70.94453249159 10.8178 9.4109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63934_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 63934_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37533_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 37533_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60161_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 60161_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93485_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 93485_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47689_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 47689_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58267_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 58267_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17856_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 17856_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108399_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 108399_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30532_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 30532_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:10:09.11 +72:28:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56057_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 56057_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63520_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 63520_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94536_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 94536_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94577_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 94577_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91576_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 91576_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111837_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 111837_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55137_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 55137_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112546_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 112546_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58845_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 58845_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95564_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 95564_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71079_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 71079_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35375_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 35375_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45630_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 45630_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:35:14.10 +70:44:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18477_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 18477_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:54:34.54 +72:29:30.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100798_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 100798_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31670_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 31670_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 01:04:32.55 +71:02:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100766_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 100766_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22175_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 22175_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125632_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 125632_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:46:46.05 +71:48:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.700 2227738689637660032 356.69131061443 +71.81204041012 12.0494 10.4212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39870_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 39870_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62544_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 62544_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13668_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 13668_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:13:10.30 +73:51:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71681_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 71681_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66618_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 66618_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 00:45:35.44 +68:37:22.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111976_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 111976_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103036_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 103036_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107881_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 107881_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100627_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 100627_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72860_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 72860_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:34:05.13 +69:11:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.205 2214064338402299008 353.51931888297 +69.19643507923 11.3273 9.7200 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44450_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 44450_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105084_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 105084_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29900_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 29900_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103223_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 103223_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69434_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 69434_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69142_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 69142_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66682_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 66682_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59911_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 59911_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87145_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
The candidate 87145_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052 did not pass the final checks
**** FOUND 23:08:04.05 +67:50:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111543_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
Preparing report for the candidate 111543_fd_Cep-03-Q2b1x1_2026-04-02_04-31-53_20.00sec_-15.00C_LIGHT_0052
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 38s
Prepared the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:54:34.61 +72:29:30.2
00:10:29.62 +67:02:32.1
00:03:34.61 +67:13:00.7
23:20:37.33 +67:32:15.1
23:58:31.29 +68:23:17.4
00:38:56.09 +68:02:34.9
00:25:47.88 +67:09:26.5
00:40:46.36 +66:59:00.4
23:37:04.79 +68:43:52.7
23:48:51.33 +68:24:36.4
00:31:25.25 +67:38:21.7
00:42:37.80 +67:20:06.9
23:47:57.71 +68:35:43.5
01:01:56.80 +69:39:31.6
00:54:22.20 +68:40:52.6
00:57:50.51 +68:13:41.2
00:47:59.72 +72:47:49.7
00:39:22.29 +72:34:14.7
00:59:30.96 +71:21:48.1
01:07:39.55 +70:34:55.3
01:03:55.88 +70:33:17.8
00:59:51.35 +70:29:37.3
00:53:50.16 +70:20:05.7
00:55:27.97 +70:00:52.5
00:38:54.20 +69:51:36.1
00:45:50.08 +69:33:37.3
00:30:24.02 +69:47:38.8
00:05:22.05 +70:09:44.2
00:50:34.62 +69:04:02.5
01:02:42.21 +68:37:31.0
00:15:55.78 +69:42:27.6
23:00:12.04 +70:02:25.4
00:55:32.73 +68:28:54.0
00:33:33.14 +68:57:42.2
00:54:15.71 +68:03:44.1
00:30:26.02 +68:42:59.1
01:00:04.55 +67:37:23.1
00:46:37.08 +68:00:53.7
00:34:42.39 +65:40:12.8
00:15:07.58 +66:20:41.0
00:37:27.36 +65:50:16.8
00:19:04.13 +66:22:15.2
00:34:08.57 +66:02:57.0
########### Completed Cep-03-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 ####
00:54:34.61 +72:29:30.2
01:01:56.80 +69:39:31.6
00:54:22.20 +68:40:52.6
00:57:50.51 +68:13:41.2
00:55:32.73 +68:28:54.0
01:03:55.88 +70:33:17.8
01:02:42.21 +68:37:31.0
00:15:07.58 +66:20:41.0
00:55:27.97 +70:00:52.5
00:30:24.02 +69:47:38.8
00:47:59.72 +72:47:49.7
23:37:04.79 +68:43:52.7
00:45:50.08 +69:33:37.3
23:00:12.04 +70:02:25.4
00:37:27.36 +65:50:16.8
00:19:04.13 +66:22:15.2
00:34:42.39 +65:40:12.8
00:31:25.25 +67:38:21.7
00:38:54.20 +69:51:36.1
23:47:57.71 +68:35:43.5
00:05:22.05 +70:09:44.2
00:34:08.57 +66:02:57.0
01:00:04.55 +67:37:23.1
01:07:39.55 +70:34:55.3
23:20:37.33 +67:32:15.1
00:03:34.61 +67:13:00.7
00:39:22.29 +72:34:14.7
00:59:51.35 +70:29:37.3
00:15:55.78 +69:42:27.6
00:46:37.08 +68:00:53.7
00:42:37.80 +67:20:06.9
23:58:31.29 +68:23:17.4
00:40:46.36 +66:59:00.4
00:10:29.62 +67:02:32.1
00:53:50.16 +70:20:05.7
00:25:47.88 +67:09:26.5
00:59:30.96 +71:21:48.1
00:38:56.09 +68:02:34.9
00:30:26.02 +68:42:59.1
00:54:15.71 +68:03:44.1
00:33:33.14 +68:57:42.2
00:50:34.62 +69:04:02.5
23:48:51.33 +68:24:36.4
###################################################################################
00:54:34.61 +72:29:30.2 -- not an asteroid (will add it to exclusion list)
01:01:56.80 +69:39:31.6 -- not an asteroid (will add it to exclusion list)
00:54:22.20 +68:40:52.6 -- not an asteroid (will add it to exclusion list)
00:57:50.51 +68:13:41.2 -- not an asteroid (will add it to exclusion list)
00:55:32.73 +68:28:54.0 -- not an asteroid (will add it to exclusion list)
01:03:55.88 +70:33:17.8 -- not an asteroid (will add it to exclusion list)
01:02:42.21 +68:37:31.0 -- not an asteroid (will add it to exclusion list)
00:15:07.58 +66:20:41.0 -- not an asteroid (will add it to exclusion list)
00:55:27.97 +70:00:52.5 -- not an asteroid (will add it to exclusion list)
00:30:24.02 +69:47:38.8 -- not an asteroid (will add it to exclusion list)
00:47:59.72 +72:47:49.7 -- not an asteroid (will add it to exclusion list)
23:37:04.79 +68:43:52.7 -- not an asteroid (will add it to exclusion list)
00:45:50.08 +69:33:37.3 -- not an asteroid (will add it to exclusion list)
23:00:12.04 +70:02:25.4 -- not an asteroid (will add it to exclusion list)
00:37:27.36 +65:50:16.8 -- not an asteroid (will add it to exclusion list)
00:19:04.13 +66:22:15.2 -- not an asteroid (will add it to exclusion list)
00:34:42.39 +65:40:12.8 -- not an asteroid (will add it to exclusion list)
00:31:25.25 +67:38:21.7 -- not an asteroid (will add it to exclusion list)
00:38:54.20 +69:51:36.1 -- not an asteroid (will add it to exclusion list)
23:47:57.71 +68:35:43.5 -- not an asteroid (will add it to exclusion list)
00:05:22.05 +70:09:44.2 -- not an asteroid (will add it to exclusion list)
00:34:08.57 +66:02:57.0 -- not an asteroid (will add it to exclusion list)
01:00:04.55 +67:37:23.1 -- not an asteroid (will add it to exclusion list)
01:07:39.55 +70:34:55.3 -- not an asteroid (will add it to exclusion list)
23:20:37.33 +67:32:15.1 -- not an asteroid (will add it to exclusion list)
00:03:34.61 +67:13:00.7 -- not an asteroid (will add it to exclusion list)
00:39:22.29 +72:34:14.7 -- not an asteroid (will add it to exclusion list)
00:59:51.35 +70:29:37.3 -- not an asteroid (will add it to exclusion list)
00:15:55.78 +69:42:27.6 -- not an asteroid (will add it to exclusion list)
00:46:37.08 +68:00:53.7 -- not an asteroid (will add it to exclusion list)
00:42:37.80 +67:20:06.9 -- not an asteroid (will add it to exclusion list)
23:58:31.29 +68:23:17.4 -- not an asteroid (will add it to exclusion list)
00:40:46.36 +66:59:00.4 -- not an asteroid (will add it to exclusion list)
00:10:29.62 +67:02:32.1 -- not an asteroid (will add it to exclusion list)
00:53:50.16 +70:20:05.7 -- not an asteroid (will add it to exclusion list)
00:25:47.88 +67:09:26.5 -- not an asteroid (will add it to exclusion list)
00:59:30.96 +71:21:48.1 -- not an asteroid (will add it to exclusion list)
00:38:56.09 +68:02:34.9 -- not an asteroid (will add it to exclusion list)
00:30:26.02 +68:42:59.1 -- not an asteroid (will add it to exclusion list)
00:54:15.71 +68:03:44.1 -- not an asteroid (will add it to exclusion list)
00:33:33.14 +68:57:42.2 -- not an asteroid (will add it to exclusion list)
00:50:34.62 +69:04:02.5 -- not an asteroid (will add it to exclusion list)
23:48:51.33 +68:24:36.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:03:34.61 +67:13:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:22.05 +70:09:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:29.62 +67:02:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:07.58 +66:20:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:55.78 +69:42:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:04.13 +66:22:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:47.88 +67:09:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:24.02 +69:47:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:26.02 +68:42:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:25.25 +67:38:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:33.14 +68:57:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:08.57 +66:02:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:42.39 +65:40:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:27.36 +65:50:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:54.20 +69:51:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:56.09 +68:02:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:22.29 +72:34:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:46.36 +66:59:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:37.80 +67:20:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:50.08 +69:33:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:37.08 +68:00:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:59.72 +72:47:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:34.62 +69:04:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:50.16 +70:20:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:15.71 +68:03:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:22.20 +68:40:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:34.61 +72:29:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:27.97 +70:00:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:32.73 +68:28:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:50.51 +68:13:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:30.96 +71:21:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:51.35 +70:29:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:04.55 +67:37:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:56.80 +69:39:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:42.21 +68:37:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:55.88 +70:33:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.55 +70:34:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:12.04 +70:02:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:37.33 +67:32:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:04.79 +68:43:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:57.71 +68:35:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:51.33 +68:24:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:31.29 +68:23:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:03:34.61 +67:13:00.7 -- a known variable star
00:05:22.05 +70:09:44.2 -- a known variable star
00:10:29.62 +67:02:32.1 -- a known variable star
00:15:07.58 +66:20:41.0 -- a known variable star
00:15:55.78 +69:42:27.6 -- a known variable star
00:19:04.13 +66:22:15.2 -- a known variable star
00:25:47.88 +67:09:26.5 -- a known variable star
00:30:24.02 +69:47:38.8 -- a known variable star
00:30:26.02 +68:42:59.1 -- a known variable star
00:31:25.25 +67:38:21.7 -- a known variable star
00:33:33.14 +68:57:42.2 -- a known variable star
00:34:08.57 +66:02:57.0 -- a known variable star
00:34:42.39 +65:40:12.8 -- a known variable star
00:37:27.36 +65:50:16.8 -- a known variable star
00:38:54.20 +69:51:36.1 -- a known variable star
00:38:56.09 +68:02:34.9 -- a known variable star
00:39:22.29 +72:34:14.7 -- a known variable star
00:40:46.36 +66:59:00.4 -- a known variable star
00:42:37.80 +67:20:06.9 -- a known variable star
00:45:50.08 +69:33:37.3 -- a known variable star
00:46:37.08 +68:00:53.7 -- a known variable star
00:47:59.72 +72:47:49.7 -- a known variable star
00:50:34.62 +69:04:02.5 -- a known variable star
00:53:50.16 +70:20:05.7 -- a known variable star
00:54:15.71 +68:03:44.1 -- a known variable star
00:54:22.20 +68:40:52.6 -- a known variable star
00:54:34.61 +72:29:30.2 -- a known variable star
00:55:27.97 +70:00:52.5 -- a known variable star
00:55:32.73 +68:28:54.0 -- a known variable star
00:57:50.51 +68:13:41.2 -- a known variable star
00:59:30.96 +71:21:48.1 -- a known variable star
00:59:51.35 +70:29:37.3 -- a known variable star
01:00:04.55 +67:37:23.1 -- a known variable star
01:01:56.80 +69:39:31.6 -- a known variable star
01:02:42.21 +68:37:31.0 -- a known variable star
01:03:55.88 +70:33:17.8 -- a known variable star
01:07:39.55 +70:34:55.3 -- a known variable star
23:00:12.04 +70:02:25.4 -- a known variable star
23:20:37.33 +67:32:15.1 -- a known variable star
23:37:04.79 +68:43:52.7 -- a known variable star
23:47:57.71 +68:35:43.5 -- a known variable star
23:48:51.33 +68:24:36.4 -- a known variable star
23:58:31.29 +68:23:17.4 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 43 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.89658183 -observatory V36
23:05:29.10 -07:28:31.6 Mercury (0.4mag)
02:03:39.64 +12:08:38.3 Venus (-3.9mag)
23:39:02.13 -03:24:00.6 Mars (1.2mag)
07:07:28.95 +22:54:15.6 Jupiter (-2.2mag)
00:23:01.79 +00:10:14.3 Saturn (0.9mag)
03:45:00.72 +19:38:45.9 Uranus (5.8mag)
00:09:00.60 -00:26:59.2 Neptune (7.8mag)
20:32:59.30 -22:52:38.0 Pluto (14.5mag)
12:51:29.91 -09:44:12.2 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461132.89658183:
07:07:36.92 +22:53:59.5 Io (5.7mag)
07:07:41.49 +22:53:51.1 Europa (5.8mag)
07:07:38.25 +22:53:50.3 Ganymede (5.3mag)
07:07:45.16 +22:53:35.1 Callisto (6.5mag)
07:11:18.66 +22:48:48.3 Himalia (15.3mag)
07:07:33.23 +22:54:06.9 Thebe (16.1mag)
07:11:10.73 +23:16:37.1 Elara (17.2mag)
07:05:26.37 +23:41:23.5 Pasiphae (17.3mag)
07:16:04.93 +22:50:41.8 Carme (18.4mag)
00:22:54.39 +00:10:39.2 Titan (8.8mag)
00:22:59.64 +00:10:21.6 Rhea (10.1mag)
00:23:11.02 +00:12:09.7 Iapetus (11.5mag)
00:22:52.22 +00:10:22.4 Hyperion (14.8mag)
00:24:48.60 +00:20:25.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.89658183:
14:22:22.30 -04:38:34.9 JWST
19:50:46.50 +04:37:38.8 Chandra
08:39:47.95 -48:22:09.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:35 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.89658183 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:46.03 -28:02:31.9 14.0mag P/2010 H2 (Vales)
04:57:45.04 -70:20:49.8 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.44 +31:21:18.6 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.79 +08:54:31.5 17.6mag C/2021 G2 (ATLAS)
23:06:06.10 +28:44:48.0 17.0mag C/2022 E2 (ATLAS)
04:13:45.71 +25:39:16.7 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.88 +31:49:52.9 16.1mag C/2022 QE78 (ATLAS)
08:29:48.60 -01:40:20.9 17.3mag C/2022 R6 (PANSTARRS)
18:56:02.37 +17:21:55.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.70 -11:42:36.4 17.6mag P/2023 B1 (PANSTARRS)
09:15:13.88 -14:09:14.0 17.5mag C/2023 F3 (ATLAS)
21:38:49.16 +62:11:20.0 17.4mag C/2023 H5 (Lemmon)
19:28:31.63 -03:34:41.8 14.3mag C/2023 R1 (PANSTARRS)
21:42:55.06 +84:09:03.5 17.8mag C/2023 X2 (Lemmon)
06:13:57.84 +63:37:27.1 17.0mag C/2024 A1 (ATLAS)
04:41:40.59 +12:46:36.4 10.1mag C/2024 E1 (Wierzchos)
16:27:03.91 +04:09:20.1 17.4mag C/2024 G6 (ATLAS)
20:16:00.61 +11:43:28.8 14.8mag C/2024 J3 (ATLAS)
03:14:34.13 -24:32:33.0 16.4mag C/2024 T5 (ATLAS)
05:05:49.26 +48:53:07.3 17.6mag C/2025 J1 (Borisov)
14:33:42.13 +33:18:37.3 14.7mag C/2025 L1 (ATLAS)
03:04:56.69 -24:13:03.3 17.7mag C/2025 Q3 (ATLAS)
22:45:39.55 +19:45:20.4 10.7mag C/2025 R3 (PANSTARRS)
13:00:01.59 +02:08:29.5 17.5mag C/2025 Y1 (ATLAS)
01:20:32.91 +02:42:01.0 8.3mag C/2026 A1 (MAPS)
23:19:07.83 +34:22:22.4 14.1mag C/2026 B2 (Sun-Gao)
18:16:21.68 -10:23:27.4 12.6mag 10P/Tempel
15:17:07.41 +04:23:49.4 12.8mag 24P/Schaumasse
11:07:06.15 -02:00:16.6 15.7mag 29P/Schwassmann-Wachmann
17:54:21.62 -10:08:56.1 17.6mag 40P/Vaisala
10:39:54.86 -05:18:40.6 16.6mag 43P/Wolf-Harrington
01:27:44.79 +15:07:50.6 17.1mag 47P/Ashbrook-Jackson
06:47:01.70 +39:51:34.8 17.1mag 63P/Wild
23:11:14.58 -13:08:04.9 15.7mag 65P/Gunn
03:28:09.56 +16:17:48.0 15.8mag 76P/West-Kohoutek-Ikemura
00:35:52.84 +05:31:36.6 14.5mag 78P/Gehrels
22:20:19.84 -13:21:45.1 14.5mag 88P/Howell
01:32:57.29 +16:51:52.5 15.1mag 93P/Lovas
04:30:23.26 +31:29:36.0 16.3mag 123P/West-Hartley
08:14:38.60 +44:38:20.4 16.2mag 124P/Mrkos
02:12:31.17 +12:48:59.8 16.4mag 128P/Shoemaker-Holt
02:21:03.90 +12:45:02.1 17.4mag 131P/Mueller
00:17:16.18 +08:06:20.0 11.6mag 141P/Machholz
00:27:26.64 -00:11:23.6 11.6mag 141P-A/Machholz
23:20:18.24 -03:34:50.4 14.5mag 141P-D/Machholz
00:55:53.70 +01:24:07.7 18.0mag 141P-I/Machholz
00:24:39.12 -08:16:33.5 15.3mag 162P/SidingSpring
10:32:23.60 +31:42:26.1 17.7mag 164P/Christensen
06:11:32.53 +24:36:02.2 17.8mag 198P/ODAS
15:15:04.77 -01:41:08.6 17.2mag 210P/Christensen
20:56:24.95 -14:43:52.3 17.3mag 218P/LINEAR
17:10:12.57 -15:29:06.8 16.2mag 235P/LINEAR
05:05:50.73 +33:28:17.4 16.5mag 240P/NEAT
07:32:51.91 -06:45:07.4 17.6mag 242P/Spahr
15:46:52.91 +06:01:50.2 17.6mag 391P/Kowalski
07:29:56.77 +21:16:34.9 17.6mag 450P/LONEOS
05:16:45.09 +45:50:21.4 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:35 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 2 04:35 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:03:36.117 -67:58:13.34 SN 2026hkg 2026-03-27.12 18.505
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
-rw-r--r-- 1 apache apache 29K Apr 2 04:35 tns_transients_list.txt
