This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF
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 20.4376* 01 12 06.82 +68 01 38.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 18 49.94 +68 31 18.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 531921460408269312,2461150.9376,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 531921460408269312 20260420.4376 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 24 27.51 +69 18 47.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 20.4376* 01 27 19.68 +69 27 08.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 09 32.16 +67 33 00.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 13 11.63 +68 33 04.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 09 09.52 +67 32 48.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 06 52.02 +67 02 45.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 16 58.97 +68 56 24.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 26 16.28 +69 21 20.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532324263922050944,2461150.9376,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532324263922050944 20260420.4376 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 00 58 44.99 +65 31 09.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J005843.55+653059.1,2461150.9376,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J005843.55+653059.1 20260420.4376 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 20.4376* 01 05 01.30 +67 20 41.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 02 03.22 +66 35 52.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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!
TCP 2026 04 20.4376* 01 07 24.05 +67 22 50.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526504789394167168,2461150.9376,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526504789394167168 20260420.4376 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 07 28.70 +67 46 10.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 26 43.95 +69 22 41.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 05 50.85 +67 10 04.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 07 07.36 +67 12 42.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526408135451167872,2461150.9376,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526408135451167872 20260420.4376 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 31 58.24 +69 49 33.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 23 22.28 +69 10 55.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 27 19.32 +69 35 38.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 18 38.89 +69 07 49.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J011838.99+690753.1,2461150.9376,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011838.99+690753.1 20260420.4376 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!
TCP 2026 04 20.4376* 00 58 12.95 +65 54 24.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525906929945680000,2461150.9376,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 525906929945680000 20260420.4376 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 15 00.88 +68 22 35.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 00 48.54 +66 56 52.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526058696910777984,2461150.9376,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526058696910777984 20260420.4376 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 20.4376* 01 16 08.28 +68 34 07.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 531936136315886336,2461150.9376,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 531936136315886336 20260420.4376 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 05 01.30 +67 37 35.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526569901099467008,2461150.9376,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526569901099467008 20260420.4376 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!
TCP 2026 04 20.4376* 01 04 39.69 +66 51 37.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526379956165106944,2461150.9376,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526379956165106944 20260420.4376 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 13 06.70 +68 09 36.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J011306.85+680936.2,2461150.9376,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011306.85+680936.2 20260420.4376 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 15 52.24 +67 39 18.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 12 16.09 +68 24 37.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 20.4376* 01 13 24.71 +68 03 09.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 13 29.29 +68 08 13.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 14 53.22 +68 36 36.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4376 2461150.9376 12.34 01:08:59.12 +67:25:14.3
124.62036 4.60643 galactic Cas Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 526503140123048192 | 01:08:59.15 +67:25:14.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.399+/-0.035 (Very red! L if it's a dwarf)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 20.4376* 01 08 59.12 +67 25 14.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 526503140123048192,2461150.9376,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 526503140123048192 20260420.4376 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 00 59 43.48 +66 19 09.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 07 54.91 +67 30 17.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 08 50.14 +67 27 15.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526506129423868544,2461150.9376,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526506129423868544 20260420.4376 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 30 53.48 +69 48 39.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 24 42.14 +69 06 58.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532296707412033280,2461150.9376,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532296707412033280 20260420.4376 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!
TCP 2026 04 20.4376* 01 05 06.37 +67 10 58.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526416141270100480,2461150.9376,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526416141270100480 20260420.4376 11.81CV 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 20.4376* 01 01 05.21 +66 51 11.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526057219442106752,2461150.9376,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526057219442106752 20260420.4376 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 12 35.14 +68 13 40.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532560246605388672,2461150.9376,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532560246605388672 20260420.4376 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 20.4376* 01 28 51.06 +69 29 15.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012851.24+692916.1,2461150.9376,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012851.24+692916.1 20260420.4376 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 01 46.86 +66 56 40.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010146.91+665640.9,2461150.9376,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010146.91+665640.9 20260420.4376 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 05 22.18 +67 15 17.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 03 40.39 +67 03 37.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 06 18.76 +67 10 50.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 12 41.35 +68 40 13.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532599794664655872,2461150.9376,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532599794664655872 20260420.4376 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 20.4376* 01 15 13.81 +68 55 47.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532700739277384448,2461150.9376,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532700739277384448 20260420.4376 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 20 46.79 +68 58 22.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.55CV 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!
TCP 2026 04 20.4376* 01 26 06.98 +69 17 33.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 10 50.67 +68 17 55.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532565087030577664,2461150.9376,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532565087030577664 20260420.4376 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 31 17.79 +69 55 05.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 532446893827763968,2461150.9376,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 532446893827763968 20260420.4376 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 13 59.53 +68 41 01.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 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 20.4376* 01 17 10.30 +68 57 19.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9376,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4376 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4376* 01 04 47.72 +67 13 48.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526416450507720320,2461150.9376,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 526416450507720320 20260420.4376 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 3
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461150.93795587 20.04.2026 10:30:29.387 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15633
Objects passed selection criteria: 15511
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 3
Average stars detected per image: 11795.3
Average stars matched: 11417 (96.7925 %)
Memory usage VmPeak: 120628 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:36:57 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## 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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461150.93795587 20.04.2026 10:30:29.387 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 98
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 42 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): 102890
Objects passed selection criteria: 102572
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 66496.2
Average stars matched: 63565.5 (95.5926 %)
Memory usage VmPeak: 1976896 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:40:24 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
Last image: 2461150.93727032 20.04.2026 10:29:30.156 UTC
ERROR running VaST on the field Cep-03-Q1b1x1 (less than 4 images processed)
exp_start= 27.12.2025 02:10:15.676 exp= 20.000 JD= 2461036.59057495 ap= 6.7 rotation= 0.000 *detected= 16537 *matched= 16537 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
exp_start= 27.12.2025 02:10:55.740 exp= 20.000 JD= 2461036.59103866 ap= 6.7 rotation= -0.011 *detected= 16611 *matched= 15630 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
exp_start= 20.04.2026 10:29:30.156 exp= 20.000 JD= 2461150.93727032 ap= 6.6 rotation= -175.257 *detected= 2823 *matched= 2642 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
exp_start= 20.04.2026 10:30:29.387 exp= 20.000 JD= 2461150.93795587 ap= 6.5 rotation= -175.265 *detected= 2238 *matched= 2084 status=OK /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.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: 2461150.93727032
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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
NOT SAVING wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
NOT SAVING wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits exists and is non-empty
NOT SAVING wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits exists and is non-empty
NOT SAVING wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits (1st reference image)
verification OK: wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:02.007 +69:59:50.87 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits (1st new image)
verification OK: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
Image size: 916.7'x605.0' 15.3(deg)x10.1(deg) 9576x6388 pix
Image scale: 5.74"/pix along the X axis and 5.68"/pix along the Y axis
Image center: 00:00:21.358 +69:59:50.50 J2000 4789.000 3195.000
###################################
###################################
# 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 00:00:21.358 +69:59:50.50
Angular distance between the image centers 0.0276 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits (2nd new image)
verification OK: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
Image size: 941.9'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:58.920 +70:01:01.27 J2000 4789.000 3195.000
###################################
###################################
# 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 23:59:58.920 +70:01:01.27
Angular distance between the image centers 0.0200 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 00:00:21.358 +69:59:50.50
Second-epoch second image center 23:59:58.920 +70:01:01.27
Angular distance between the image centers 0.03753 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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.EObkpXfWv1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.5k68gjrrGW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits &> /tmp/tmp.ysVElZgV3d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits &> /tmp/tmp.yxuvBBXkso
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q1b1x1_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.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 66 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.3 pix Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.6 pix fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
2.5 pix fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
Limiting magnitude estimates:
15.2 mag. Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.2 mag. Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
13.4 mag. fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
12.8 mag. fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EObkpXfWv1 (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q1b1x1_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-Q1b1x1_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...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 112172 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 112171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 112171 with non-zero local correction accuracy
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q1b1x1_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-Q1b1x1_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.5k68gjrrGW (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q1b1x1_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=50, blended=12319, passed=113219
Got 113219 stars (including 100702 good ones) from the SExtractor catalog wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 113219 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 348 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 300 matched stars entering correct_measured_positions(), 255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.20"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 296 matched stars entering correct_measured_positions(), 28117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.65"
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 332.7175 through 0 to 27.8814, gap 27.8814 to 332.7175
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 411 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 386 matched stars entering correct_measured_positions(), 28142 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.63"
Accuracy estimation diagnostic: 386 matched stars entering correct_measured_positions(), 35135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.63"
Excluding outliers - 386 stars left (next iteration limit 325)
The image catalog is written to wcs_Cep-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q1b1x1_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-Q1b1x1_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.ysVElZgV3d (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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=745, passed=22396
Got 22396 stars (including 21607 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 22396 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 916.7'
Seting catalog search parameters based on the expected field of view 916.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012732 (45.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010186 (36.7 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 334.4671 through 0 to 28.4273, gap 28.4273 to 334.4671
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 735 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 709 matched stars entering correct_measured_positions(), 673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 708 matched stars entering correct_measured_positions(), 14859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.24"
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 334.4694 through 0 to 28.4237, gap 28.4237 to 334.4694
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 736 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 721 matched stars entering correct_measured_positions(), 14867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.19"
Accuracy estimation diagnostic: 721 matched stars entering correct_measured_positions(), 14974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.13"
Excluding outliers - 721 stars left (next iteration limit 778)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits -region wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.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.yxuvBBXkso (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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.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_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=515, passed=18848
Got 18848 stars (including 18290 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 18848 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.0395 through 0 to 28.4209, gap 28.4209 to 332.0395
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 17794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 332.0380 through 0 to 28.4224, gap 28.4224 to 332.0380
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 17793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 17793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits -region wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.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-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/wcs_Cep-03-Q1b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_Cep-03-Q1b1x1_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-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/wcs_Cep-03-Q1b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-29-30_20.00sec_-4.90C_LIGHTs_0020.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cep-03-Q1b1x1_053128_TTUQ1b1x1_3207762_KeaUYCsF/wcs_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021.fits'
Preparing the HTML report for the field Cep-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_local.txt__out102829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99368.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 110s
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: 35s
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Considering the candidate 134505_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 134505_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 01:47:58.16 +72:17:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134740_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 134740_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 00:36:26.63 +70:47:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134777_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 134777_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 00:36:37.97 +68:42:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134821_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 134821_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 01:32:21.00 +70:01:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135145_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 135145_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 00:49:34.93 +70:27:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135370_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 135370_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 00:38:43.62 +71:10:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62279_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 62279_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 54068_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 54068_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 42002_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 42002_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 38737_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 38737_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 68251_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 68251_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 56471_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 56471_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 68418_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 68418_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 102829_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 102829_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 50476_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 50476_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 40440_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 40440_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 99368_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 99368_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 71728_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 71728_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 111688_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 111688_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 70547_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 70547_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 66972_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 66972_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 39869_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 39869_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 72945_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72945_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 72098_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72098_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 31949_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 31949_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 43975_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 43975_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 37185_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 37185_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 47286_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 47286_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 103282_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 103282_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 09055_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 09055_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (2126.7") between the two second-epoch detections
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Considering the candidate 57378_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 57378_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 111995_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 111995_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 54902_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 54902_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69311_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 69311_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 111621_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 111621_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 60357_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 60357_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 64450_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 64450_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58228_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 58228_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61498_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 61498_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60548_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 60548_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55022_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 55022_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 69718_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 69718_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45630_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 45630_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 00:35:14.55 +70:44:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107739_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 107739_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69343_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 69343_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 71428_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
The candidate 71428_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 01:02:57.23 +67:26:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69423_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 69423_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 32709_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 32709_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 44217_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 44217_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72991_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72991_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 113803_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 113803_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 60016_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 60016_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 37521_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 37521_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 112079_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 112079_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 72406_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72406_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 106394_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 106394_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 72656_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72656_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 55346_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 55346_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51310_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 51310_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48017_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 48017_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41300_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 41300_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 60034_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 60034_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31321_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 31321_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54723_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 54723_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50209_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 50209_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72814_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 72814_fd_Cep-03-Q1b1x1_2026-04-20_05-30-29_20.00sec_-5.00C_LIGHTs_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 147s
Prepared the HTML report for the field Cep-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:06:52.02 +67:02:45.5
00:58:12.95 +65:54:24.8
01:03:40.39 +67:03:37.4
00:59:43.48 +66:19:09.2
01:04:39.69 +66:51:37.5
01:02:03.22 +66:35:52.9
01:00:48.54 +66:56:52.2
01:01:46.86 +66:56:40.5
01:01:05.21 +66:51:11.3
01:31:17.79 +69:55:05.3
01:31:58.24 +69:49:33.2
01:30:53.48 +69:48:39.0
01:27:19.32 +69:35:38.6
01:28:51.06 +69:29:15.4
01:27:19.68 +69:27:08.6
01:26:43.95 +69:22:41.5
01:26:16.28 +69:21:20.5
01:26:06.98 +69:17:33.8
01:24:27.51 +69:18:47.1
01:23:22.28 +69:10:55.0
01:24:42.14 +69:06:58.6
01:18:38.89 +69:07:49.8
01:20:46.79 +68:58:22.6
01:17:10.30 +68:57:19.1
01:16:58.97 +68:56:24.2
01:15:13.81 +68:55:47.7
01:18:49.94 +68:31:18.4
01:13:59.53 +68:41:01.4
01:16:08.28 +68:34:07.6
01:14:53.22 +68:36:36.2
01:12:41.35 +68:40:13.6
01:13:11.63 +68:33:04.6
01:15:00.88 +68:22:35.0
01:12:16.09 +68:24:37.9
01:12:35.14 +68:13:40.9
01:10:50.67 +68:17:55.4
01:13:06.70 +68:09:36.3
01:13:29.29 +68:08:13.0
01:13:24.71 +68:03:09.9
01:12:06.82 +68:01:38.9
01:15:52.24 +67:39:18.3
01:07:28.70 +67:46:10.7
01:09:32.16 +67:33:00.8
01:09:09.52 +67:32:48.4
01:05:01.30 +67:37:35.2
01:07:54.91 +67:30:17.6
01:08:50.14 +67:27:15.1
01:08:59.12 +67:25:14.3
01:07:24.05 +67:22:50.6
01:05:01.30 +67:20:41.7
01:07:07.36 +67:12:42.2
01:05:22.18 +67:15:17.6
01:06:18.76 +67:10:50.6
01:04:47.72 +67:13:48.6
01:05:50.85 +67:10:04.7
01:05:06.37 +67:10:58.0
00:58:44.99 +65:31:09.1
########### Completed Cep-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:12:06.82 +68:01:38.9
01:18:49.94 +68:31:18.4
01:24:27.51 +69:18:47.1
01:27:19.68 +69:27:08.6
01:09:32.16 +67:33:00.8
01:13:11.63 +68:33:04.6
01:09:09.52 +67:32:48.4
01:06:52.02 +67:02:45.5
01:16:58.97 +68:56:24.2
01:26:16.28 +69:21:20.5
00:58:44.99 +65:31:09.1
01:05:01.30 +67:20:41.7
01:02:03.22 +66:35:52.9
01:07:24.05 +67:22:50.6
01:07:28.70 +67:46:10.7
01:26:43.95 +69:22:41.5
01:05:50.85 +67:10:04.7
01:07:07.36 +67:12:42.2
01:31:58.24 +69:49:33.2
01:23:22.28 +69:10:55.0
01:27:19.32 +69:35:38.6
01:18:38.89 +69:07:49.8
00:58:12.95 +65:54:24.8
01:15:00.88 +68:22:35.0
01:00:48.54 +66:56:52.2
01:16:08.28 +68:34:07.6
01:05:01.30 +67:37:35.2
01:04:39.69 +66:51:37.5
01:13:06.70 +68:09:36.3
01:15:52.24 +67:39:18.3
01:12:16.09 +68:24:37.9
01:13:24.71 +68:03:09.9
01:13:29.29 +68:08:13.0
01:14:53.22 +68:36:36.2
01:08:59.12 +67:25:14.3
00:59:43.48 +66:19:09.2
01:07:54.91 +67:30:17.6
01:08:50.14 +67:27:15.1
01:30:53.48 +69:48:39.0
01:24:42.14 +69:06:58.6
01:05:06.37 +67:10:58.0
01:01:05.21 +66:51:11.3
01:12:35.14 +68:13:40.9
01:28:51.06 +69:29:15.4
01:01:46.86 +66:56:40.5
01:05:22.18 +67:15:17.6
01:03:40.39 +67:03:37.4
01:06:18.76 +67:10:50.6
01:12:41.35 +68:40:13.6
01:15:13.81 +68:55:47.7
01:20:46.79 +68:58:22.6
01:26:06.98 +69:17:33.8
01:10:50.67 +68:17:55.4
01:31:17.79 +69:55:05.3
01:13:59.53 +68:41:01.4
01:17:10.30 +68:57:19.1
01:04:47.72 +67:13:48.6
###################################################################################
01:12:06.82 +68:01:38.9 -- not an asteroid (will add it to exclusion list)
01:18:49.94 +68:31:18.4 -- not an asteroid (will add it to exclusion list)
01:24:27.51 +69:18:47.1 -- not an asteroid (will add it to exclusion list)
01:27:19.68 +69:27:08.6 -- not an asteroid (will add it to exclusion list)
01:09:32.16 +67:33:00.8 -- not an asteroid (will add it to exclusion list)
01:13:11.63 +68:33:04.6 -- not an asteroid (will add it to exclusion list)
01:09:09.52 +67:32:48.4 -- not an asteroid (will add it to exclusion list)
01:06:52.02 +67:02:45.5 -- not an asteroid (will add it to exclusion list)
01:16:58.97 +68:56:24.2 -- not an asteroid (will add it to exclusion list)
01:26:16.28 +69:21:20.5 -- not an asteroid (will add it to exclusion list)
00:58:44.99 +65:31:09.1 -- not an asteroid (will add it to exclusion list)
01:05:01.30 +67:20:41.7 -- not an asteroid (will add it to exclusion list)
01:02:03.22 +66:35:52.9 -- not an asteroid (will add it to exclusion list)
01:07:24.05 +67:22:50.6 -- not an asteroid (will add it to exclusion list)
01:07:28.70 +67:46:10.7 -- not an asteroid (will add it to exclusion list)
01:26:43.95 +69:22:41.5 -- not an asteroid (will add it to exclusion list)
01:05:50.85 +67:10:04.7 -- not an asteroid (will add it to exclusion list)
01:07:07.36 +67:12:42.2 -- not an asteroid (will add it to exclusion list)
01:31:58.24 +69:49:33.2 -- not an asteroid (will add it to exclusion list)
01:23:22.28 +69:10:55.0 -- not an asteroid (will add it to exclusion list)
01:27:19.32 +69:35:38.6 -- not an asteroid (will add it to exclusion list)
01:18:38.89 +69:07:49.8 -- not an asteroid (will add it to exclusion list)
00:58:12.95 +65:54:24.8 -- not an asteroid (will add it to exclusion list)
01:15:00.88 +68:22:35.0 -- not an asteroid (will add it to exclusion list)
01:00:48.54 +66:56:52.2 -- not an asteroid (will add it to exclusion list)
01:16:08.28 +68:34:07.6 -- not an asteroid (will add it to exclusion list)
01:05:01.30 +67:37:35.2 -- not an asteroid (will add it to exclusion list)
01:04:39.69 +66:51:37.5 -- not an asteroid (will add it to exclusion list)
01:13:06.70 +68:09:36.3 -- not an asteroid (will add it to exclusion list)
01:15:52.24 +67:39:18.3 -- not an asteroid (will add it to exclusion list)
01:12:16.09 +68:24:37.9 -- not an asteroid (will add it to exclusion list)
01:13:24.71 +68:03:09.9 -- not an asteroid (will add it to exclusion list)
01:13:29.29 +68:08:13.0 -- not an asteroid (will add it to exclusion list)
01:14:53.22 +68:36:36.2 -- not an asteroid (will add it to exclusion list)
01:08:59.12 +67:25:14.3 -- not an asteroid (will add it to exclusion list)
00:59:43.48 +66:19:09.2 -- not an asteroid (will add it to exclusion list)
01:07:54.91 +67:30:17.6 -- not an asteroid (will add it to exclusion list)
01:08:50.14 +67:27:15.1 -- not an asteroid (will add it to exclusion list)
01:30:53.48 +69:48:39.0 -- not an asteroid (will add it to exclusion list)
01:24:42.14 +69:06:58.6 -- not an asteroid (will add it to exclusion list)
01:05:06.37 +67:10:58.0 -- not an asteroid (will add it to exclusion list)
01:01:05.21 +66:51:11.3 -- not an asteroid (will add it to exclusion list)
01:12:35.14 +68:13:40.9 -- not an asteroid (will add it to exclusion list)
01:28:51.06 +69:29:15.4 -- not an asteroid (will add it to exclusion list)
01:01:46.86 +66:56:40.5 -- not an asteroid (will add it to exclusion list)
01:05:22.18 +67:15:17.6 -- not an asteroid (will add it to exclusion list)
01:03:40.39 +67:03:37.4 -- not an asteroid (will add it to exclusion list)
01:06:18.76 +67:10:50.6 -- not an asteroid (will add it to exclusion list)
01:12:41.35 +68:40:13.6 -- not an asteroid (will add it to exclusion list)
01:15:13.81 +68:55:47.7 -- not an asteroid (will add it to exclusion list)
01:20:46.79 +68:58:22.6 -- not an asteroid (will add it to exclusion list)
01:26:06.98 +69:17:33.8 -- not an asteroid (will add it to exclusion list)
01:10:50.67 +68:17:55.4 -- not an asteroid (will add it to exclusion list)
01:31:17.79 +69:55:05.3 -- not an asteroid (will add it to exclusion list)
01:13:59.53 +68:41:01.4 -- not an asteroid (will add it to exclusion list)
01:17:10.30 +68:57:19.1 -- not an asteroid (will add it to exclusion list)
01:04:47.72 +67:13:48.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:58:12.95 +65:54:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:44.99 +65:31:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:43.48 +66:19:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:48.54 +66:56:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:05.21 +66:51:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:46.86 +66:56:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:03.22 +66:35:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:40.39 +67:03:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:39.69 +66:51:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:47.72 +67:13:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:01.30 +67:20:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:01.30 +67:37:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:06.37 +67:10:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:22.18 +67:15:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:50.85 +67:10:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:18.76 +67:10:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:52.02 +67:02:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:07.36 +67:12:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:24.05 +67:22:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:28.70 +67:46:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:54.91 +67:30:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:50.14 +67:27:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.12 +67:25:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:09.52 +67:32:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:32.16 +67:33:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:50.67 +68:17:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:06.82 +68:01:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:16.09 +68:24:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:35.14 +68:13:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.35 +68:40:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:06.70 +68:09:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:11.63 +68:33:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:24.71 +68:03:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:29.29 +68:08:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:59.53 +68:41:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:53.22 +68:36:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:00.88 +68:22:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:13.81 +68:55:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:52.24 +67:39:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:08.28 +68:34:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:58.97 +68:56:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:10.30 +68:57:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:38.89 +69:07:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:49.94 +68:31:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:46.79 +68:58:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:22.28 +69:10:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:27.51 +69:18:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:42.14 +69:06:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:06.98 +69:17:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:16.28 +69:21:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:43.95 +69:22:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:19.32 +69:35:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:19.68 +69:27:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:51.06 +69:29:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:53.48 +69:48:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:17.79 +69:55:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:58.24 +69:49:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:58:12.95 +65:54:24.8 -- not a known variable star
00:58:44.99 +65:31:09.1 -- a known variable star
00:59:43.48 +66:19:09.2 -- not a known variable star
01:00:48.54 +66:56:52.2 -- not a known variable star
01:01:05.21 +66:51:11.3 -- not a known variable star
01:01:46.86 +66:56:40.5 -- a known variable star
01:02:03.22 +66:35:52.9 -- not a known variable star
01:03:40.39 +67:03:37.4 -- not a known variable star
01:04:39.69 +66:51:37.5 -- not a known variable star
01:04:47.72 +67:13:48.6 -- a known variable star
01:05:01.30 +67:20:41.7 -- not a known variable star
01:05:01.30 +67:37:35.2 -- not a known variable star
01:05:06.37 +67:10:58.0 -- not a known variable star
01:05:22.18 +67:15:17.6 -- not a known variable star
01:05:50.85 +67:10:04.7 -- not a known variable star
01:06:18.76 +67:10:50.6 -- not a known variable star
01:06:52.02 +67:02:45.5 -- not a known variable star
01:07:07.36 +67:12:42.2 -- a known variable star
01:07:24.05 +67:22:50.6 -- not a known variable star
01:07:28.70 +67:46:10.7 -- not a known variable star
01:07:54.91 +67:30:17.6 -- not a known variable star
01:08:50.14 +67:27:15.1 -- not a known variable star
01:08:59.12 +67:25:14.3 -- not a known variable star
01:09:09.52 +67:32:48.4 -- not a known variable star
01:09:32.16 +67:33:00.8 -- not a known variable star
01:10:50.67 +68:17:55.4 -- not a known variable star
01:12:06.82 +68:01:38.9 -- not a known variable star
01:12:16.09 +68:24:37.9 -- not a known variable star
01:12:35.14 +68:13:40.9 -- a known variable star
01:12:41.35 +68:40:13.6 -- not a known variable star
01:13:06.70 +68:09:36.3 -- a known variable star
01:13:11.63 +68:33:04.6 -- not a known variable star
01:13:24.71 +68:03:09.9 -- not a known variable star
01:13:29.29 +68:08:13.0 -- not a known variable star
01:13:59.53 +68:41:01.4 -- not a known variable star
01:14:53.22 +68:36:36.2 -- not a known variable star
01:15:00.88 +68:22:35.0 -- not a known variable star
01:15:13.81 +68:55:47.7 -- not a known variable star
01:15:52.24 +67:39:18.3 -- not a known variable star
01:16:08.28 +68:34:07.6 -- a known variable star
01:16:58.97 +68:56:24.2 -- not a known variable star
01:17:10.30 +68:57:19.1 -- not a known variable star
01:18:38.89 +69:07:49.8 -- a known variable star
01:18:49.94 +68:31:18.4 -- a known variable star
01:20:46.79 +68:58:22.6 -- not a known variable star
01:23:22.28 +69:10:55.0 -- not a known variable star
01:24:27.51 +69:18:47.1 -- not a known variable star
01:24:42.14 +69:06:58.6 -- a known variable star
01:26:06.98 +69:17:33.8 -- not a known variable star
01:26:16.28 +69:21:20.5 -- a known variable star
01:26:43.95 +69:22:41.5 -- not a known variable star
01:27:19.32 +69:35:38.6 -- not a known variable star
01:27:19.68 +69:27:08.6 -- not a known variable star
01:28:51.06 +69:29:15.4 -- a known variable star
01:30:53.48 +69:48:39.0 -- not a known variable star
01:31:17.79 +69:55:05.3 -- not a known variable star
01:31:58.24 +69:49:33.2 -- not a known variable star
Found 45 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
57 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 57 (excluding asteroids and hot pixels, 45 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461150.93727032 -observatory V36
00:31:41.07 +00:34:26.6 Mercury (-0.1mag)
03:30:31.94 +19:26:31.3 Venus (-3.9mag)
00:30:26.16 +02:14:47.0 Mars (1.2mag)
07:14:45.02 +22:42:40.4 Jupiter (-2.1mag)
00:31:08.67 +01:01:10.0 Saturn (0.9mag)
03:48:38.90 +19:50:30.4 Uranus (5.8mag)
00:11:24.78 -00:11:46.5 Neptune (7.8mag)
20:33:55.78 -22:52:52.6 Pluto (14.5mag)
04:35:02.46 +26:15:51.0 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 362 Apr 20 05:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461150.93727032:
07:14:47.01 +22:42:33.6 Io (5.8mag)
07:14:57.44 +22:42:12.7 Europa (5.9mag)
07:14:38.46 +22:43:01.0 Ganymede (5.4mag)
07:14:44.72 +22:42:31.6 Callisto (6.6mag)
07:17:53.00 +22:28:19.1 Himalia (15.4mag)
07:14:45.17 +22:42:42.3 Thebe (16.3mag)
07:18:09.72 +22:58:39.2 Elara (17.3mag)
07:13:56.02 +23:20:21.4 Pasiphae (17.4mag)
07:22:58.59 +22:41:06.4 Carme (18.5mag)
00:30:59.36 +01:01:22.9 Titan (8.8mag)
00:31:06.17 +01:01:16.2 Rhea (10.1mag)
00:30:42.40 +01:00:36.8 Iapetus (11.5mag)
00:31:00.62 +01:01:35.3 Hyperion (14.8mag)
00:32:41.93 +01:09:28.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 20 05:40 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461150.93727032:
15:55:29.61 -19:14:04.3 JWST
18:32:14.94 +26:44:43.5 Chandra
09:07:25.41 -52:03:09.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 20 05:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461150.93727032 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:35.75 -29:02:51.7 13.9mag P/2010 H2 (Vales)
05:10:00.60 -69:27:27.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:27.63 +31:28:07.8 17.2mag C/2017 K2 (PANSTARRS)
17:29:53.61 +11:04:01.5 17.6mag C/2021 G2 (ATLAS)
23:11:19.94 +29:24:38.3 17.1mag C/2022 E2 (ATLAS)
04:34:26.98 +26:09:21.5 16.1mag C/2022 N2 (PANSTARRS)
09:04:30.30 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:31:51.40 +00:18:18.9 17.4mag C/2022 R6 (PANSTARRS)
18:52:33.75 +18:53:57.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:09.67 -11:27:22.3 17.5mag P/2023 B1 (PANSTARRS)
09:05:44.53 -11:11:13.7 17.7mag C/2023 F3 (ATLAS)
21:58:26.51 +63:10:31.6 17.5mag C/2023 H5 (Lemmon)
19:15:01.56 -03:49:01.3 14.1mag C/2023 R1 (PANSTARRS)
21:19:58.05 +86:32:05.0 17.8mag C/2023 X2 (Lemmon)
06:20:14.46 +63:30:01.7 17.2mag C/2024 A1 (ATLAS)
05:22:33.86 +19:41:09.2 11.3mag C/2024 E1 (Wierzchos)
16:16:18.68 +07:06:48.3 17.3mag C/2024 G6 (ATLAS)
20:21:54.83 +16:29:49.8 14.5mag C/2024 J3 (ATLAS)
03:30:24.12 -21:43:19.8 16.3mag C/2024 T5 (ATLAS)
05:20:32.69 +44:12:53.3 17.7mag C/2025 J1 (Borisov)
13:20:38.77 +48:00:36.3 15.4mag C/2025 L1 (ATLAS)
03:32:26.78 -26:55:25.8 17.9mag C/2025 Q3 (ATLAS)
00:36:14.05 +16:01:03.3 8.0mag C/2025 R3 (PANSTARRS)
12:52:13.12 +03:16:26.2 17.4mag C/2025 Y1 (ATLAS)
03:59:44.02 +02:14:21.7 14.5mag C/2026 A1 (MAPS)
00:11:55.63 +37:59:52.3 14.7mag C/2026 B2 (Sun-Gao)
18:51:33.15 -09:28:41.4 11.6mag 10P/Tempel
14:54:14.10 +02:43:00.7 14.4mag 24P/Schaumasse
11:01:42.72 -01:23:24.1 15.7mag 29P/Schwassmann-Wachmann
10:37:36.80 -03:46:02.5 17.0mag 43P/Wolf-Harrington
01:55:33.63 +18:14:16.1 17.3mag 47P/Ashbrook-Jackson
07:19:06.43 +36:02:47.8 17.0mag 63P/Wild
23:34:39.09 -10:55:33.2 15.7mag 65P/Gunn
04:15:16.72 +22:44:18.7 15.9mag 76P/West-Kohoutek-Ikemura
01:15:26.52 +09:05:40.0 14.3mag 78P/Gehrels
23:16:14.95 -08:04:42.6 14.7mag 88P/Howell
02:23:06.18 +21:47:59.8 15.1mag 93P/Lovas
05:03:19.60 +32:30:44.8 16.1mag 123P/West-Hartley
08:33:49.94 +36:18:59.0 16.2mag 124P/Mrkos
02:40:07.05 +14:51:31.4 16.4mag 128P/Shoemaker-Holt
02:56:16.40 +15:01:17.9 17.5mag 131P/Mueller
01:49:45.01 +14:41:26.5 10.5mag 141P/Machholz
01:57:58.94 +06:31:28.0 10.5mag 141P-A/Machholz
00:41:20.40 +02:18:31.9 12.3mag 141P-D/Machholz
02:28:33.83 +08:16:26.0 17.9mag 141P-I/Machholz
01:14:48.42 +00:42:48.9 15.0mag 162P/SidingSpring
14:43:35.87 +00:21:10.7 17.8mag 210P/Christensen
21:51:17.88 -10:23:15.8 17.7mag 218P/LINEAR
17:17:17.37 -13:23:35.9 16.1mag 235P/LINEAR
05:44:09.32 +35:00:29.1 16.8mag 240P/NEAT
07:40:48.37 -04:42:11.0 17.8mag 242P/Spahr
22:28:00.90 -19:45:56.0 17.8mag 260P/McNaught
02:07:21.57 +21:34:12.0 18.0mag 295P/LINEAR
15:40:47.61 +07:16:15.0 17.5mag 391P/Kowalski
07:36:01.38 +21:22:23.3 17.7mag 450P/LONEOS
05:42:25.93 +44:46:23.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 20 05:40 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 20 05:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:06:25.223 +11:52:09.71 AT 2026jkh 2026-04-12.15 19.52
16:50:00.163 +35:59:45.01 AT 2026jkg 2026-04-12.14 19.01
15:43:54.016 +44:51:51.60 SN 2026jkf 2026-04-12.14 18.53
11:24:19.761 -36:04:17.66 AT 2026jke 2026-04-06.51 19.98
11:16:25.694 -50:15:29.19 AT 2026jkd 2026-03-28.49 19.6
11:43:56.670 -49:03:17.42 AT 2026jkc 2026-04-12.46 19.35
11:38:21.891 -50:43:06.73 SN 2026jkb 2026-04-12.46 18.57
08:19:14.303 -28:43:36.53 AT 2026jka 2026-04-11.37 19.87
07:49:32.473 -24:44:26.65 AT 2026jjz 2026-04-12.39 18.98
14:44:18.498 -44:01:13.70 AT 2026jjy 2026-04-09.61 19.64
08:53:40.997 -38:26:31.85 AT 2026jjx 2026-03-23.40 20
12:26:02.763 -33:38:07.00 AT 2026jjw 2026-04-09.56 20.25
11:26:18.195 +19:38:31.94 AT 2026jjv 2026-04-06.91 19.81
11:33:29.132 -27:21:16.23 AT 2026jju 2026-04-12.45 19.32
12:15:03.964 -49:33:10.66 AT 2026jjt 2026-04-12.17 19.263
17:17:54.158 -75:07:32.46 AT 2026jjs 2026-04-12.30 19.194
08:35:23.434 +10:31:04.49 AT 2026jjr 2026-04-11.93 19.882
09:53:48.141 +08:12:51.52 AT 2026jjq 2026-04-11.92 20.219
12:47:33.422 +00:05:56.15 AT 2026jjp 2026-04-12.03 20.061
16:10:20.836 -68:49:59.48 AT 2026jjo 2026-04-12.26 19.161
-rw-r--r-- 1 apache apache 30K Apr 20 05:40 tns_transients_list.txt
