This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq
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 06.0858* 00 51 33.87 +68 35 26.3 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208951712415231872,2461136.5858,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208951712415231872 20260406.0858 9.47CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211955165863382016,2461136.5858,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211955165863382016 20260406.0858 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208845953138151936,2461136.5858,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208845953138151936 20260406.0858 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 45 10.92 +72 45 23.8 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2210080940914272000,2461136.5858,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2210080940914272000 20260406.0858 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 55 43.67 +70 46 36.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.10CV 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 06.0858* 00 51 52.60 +65 50 58.4 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 01 24 23.11 +72 27 05.6 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2213063404863676032,2461136.5858,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2213063404863676032 20260406.0858 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2226692122068075392,2461136.5858,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2226692122068075392 20260406.0858 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 01 06 41.04 +72 08 23.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208954186316752128,2461136.5858,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208954186316752128 20260406.0858 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2210237144585571456,2461136.5858,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2210237144585571456 20260406.0858 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208980432853176832,2461136.5858,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208980432853176832 20260406.0858 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2212331370638569600,2461136.5858,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212331370638569600 20260406.0858 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208925976970811520,2461136.5858,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208925976970811520 20260406.0858 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 01 24 17.31 +72 58 58.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2212168986513982976,2461136.5858,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212168986513982976 20260406.0858 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208885123241206144,2461136.5858,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208885123241206144 20260406.0858 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211878990322601216,2461136.5858,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211878990322601216 20260406.0858 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211880811389595136,2461136.5858,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211880811389595136 20260406.0858 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211958601836132864,2461136.5858,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211958601836132864 20260406.0858 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208899210733802496,2461136.5858,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208899210733802496 20260406.0858 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2225386726892126336,2461136.5858,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2225386726892126336 20260406.0858 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208950097507556736,2461136.5858,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208950097507556736 20260406.0858 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208853752799113600,2461136.5858,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208853752799113600 20260406.0858 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211898364916485760,2461136.5858,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211898364916485760 20260406.0858 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J225950.96+662119.3,2461136.5858,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J225950.96+662119.3 20260406.0858 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208947761045407232,2461136.5858,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208947761045407232 20260406.0858 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208841039696201984,2461136.5858,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208841039696201984 20260406.0858 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211880261632897536,2461136.5858,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211880261632897536 20260406.0858 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208860345570210944,2461136.5858,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208860345570210944 20260406.0858 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211883628886865024,2461136.5858,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211883628886865024 20260406.0858 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211896479429352576,2461136.5858,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211896479429352576 20260406.0858 11.39CV 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 06.0858* 23 53 48.16 +65 48 47.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208869970591119360,2461136.5858,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208869970591119360 20260406.0858 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208868802364464128,2461136.5858,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208868802364464128 20260406.0858 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208869283400806144,2461136.5858,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208869283400806144 20260406.0858 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208894022413331968,2461136.5858,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208894022413331968 20260406.0858 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208949925708868864,2461136.5858,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208949925708868864 20260406.0858 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211889225225741184,2461136.5858,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211889225225741184 20260406.0858 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211883796387076224,2461136.5858,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211883796387076224 20260406.0858 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208847361887775104,2461136.5858,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208847361887775104 20260406.0858 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208898798416891648,2461136.5858,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208898798416891648 20260406.0858 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.0858 2461136.5858 11.76 23:01:30.01 +65:31:21.1
111.86464 5.04092 galactic Cep Second-epoch detections are separated by 5.0" and 2.7 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 2211870915780376448 | 23:01:33.11 +65:31:17.8 (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)
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2211870915780376448,2461136.5858,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2211870915780376448 20260406.0858 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211899743604465792,2461136.5858,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211899743604465792 20260406.0858 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208849973227912832,2461136.5858,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208849973227912832 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2210473505226069760,2461136.5858,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2210473505226069760 20260406.0858 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208802350631700096,2461136.5858,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208802350631700096 20260406.0858 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211876378982624000,2461136.5858,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211876378982624000 20260406.0858 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230620.52+653731.0,2461136.5858,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230620.52+653731.0 20260406.0858 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208847980363062016,2461136.5858,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208847980363062016 20260406.0858 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208896526376153088,2461136.5858,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208896526376153088 20260406.0858 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208945665101371904,2461136.5858,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208945665101371904 20260406.0858 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208698893461568896,2461136.5858,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208698893461568896 20260406.0858 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208884917082795648,2461136.5858,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208884917082795648 20260406.0858 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211938192151685632,2461136.5858,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211938192151685632 20260406.0858 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208895568601570688,2461136.5858,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208895568601570688 20260406.0858 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208874093765368832,2461136.5858,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208874093765368832 20260406.0858 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211893588910934784,2461136.5858,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211893588910934784 20260406.0858 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211944205105833088,2461136.5858,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211944205105833088 20260406.0858 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208795375603358080,2461136.5858,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208795375603358080 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2214931367740466688,2461136.5858,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2214931367740466688 20260406.0858 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211943036874733184,2461136.5858,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211943036874733184 20260406.0858 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211873282307200128,2461136.5858,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211873282307200128 20260406.0858 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 01 15 12.88 +72 49 34.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2212369475588154880,2461136.5858,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212369475588154880 20260406.0858 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208874780958882304,2461136.5858,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208874780958882304 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208845742680876032,2461136.5858,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208845742680876032 20260406.0858 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211874145599463296,2461136.5858,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211874145599463296 20260406.0858 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208841898689095808,2461136.5858,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208841898689095808 20260406.0858 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208849625331309568,2461136.5858,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208849625331309568 20260406.0858 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208869695717647232,2461136.5858,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208869695717647232 20260406.0858 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J231001.84+651653.6,2461136.5858,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J231001.84+651653.6 20260406.0858 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208864881055139968,2461136.5858,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208864881055139968 20260406.0858 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 06.0858* 01 15 42.20 +72 48 33.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2213911918603023360,2461136.5858,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2213911918603023360 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211868403224288896,2461136.5858,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211868403224288896 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211872492033153536,2461136.5858,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211872492033153536 20260406.0858 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208895392505131264,2461136.5858,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208895392505131264 20260406.0858 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208861002705058560,2461136.5858,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208861002705058560 20260406.0858 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 36 10.56 +72 49 47.2 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211893588910934784,2461136.5858,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211893588910934784 20260406.0858 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 531237053078765312,2461136.5858,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 531237053078765312 20260406.0858 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2225754311669055488,2461136.5858,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2225754311669055488 20260406.0858 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208873647087837696,2461136.5858,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208873647087837696 20260406.0858 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2214177210143764992,2461136.5858,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2214177210143764992 20260406.0858 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230141.70+653201.9,2461136.5858,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230141.70+653201.9 20260406.0858 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208886635069913728,2461136.5858,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208886635069913728 20260406.0858 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211957154428830592,2461136.5858,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211957154428830592 20260406.0858 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.0858* 00 36 58.95 +71 06 57.4 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208870138095107968,2461136.5858,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208870138095107968 20260406.0858 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211075419121286272,2461136.5858,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211075419121286272 20260406.0858 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2212047314381087616,2461136.5858,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212047314381087616 20260406.0858 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211866105420386816,2461136.5858,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211866105420386816 20260406.0858 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 31 51.42 +69 56 50.3 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 36 49.52 +71 09 00.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 27 50.91 +68 14 03.8 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 10.47CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.0858* 00 33 38.91 +70 41 55.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230015.68+663615.8,2461136.5858,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230015.68+663615.8 20260406.0858 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.0858* 01 01 57.06 +70 59 43.4 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5858,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0858 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1301,2461136.5858,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1301 20260406.0858 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461136.58607076 06.04.2026 02:03:46.514 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
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: 4 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): 13478
Objects passed selection criteria: 13384
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 8928.25
Average stars matched: 8630.25 (96.6623 %)
Memory usage VmPeak: 119076 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:05:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461136.58607076 06.04.2026 02:03:46.514 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 283
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 19 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): 90546
Objects passed selection criteria: 90364
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 66091.8
Average stars matched: 63147.2 (95.5448 %)
Memory usage VmPeak: 1866280 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:14:54 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.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: 2461136.58555345
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits'
wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:23.610 +69:58:22.65
Angular distance between the image centers 0.0600 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:21.829 +69:58:08.10
Angular distance between the image centers 0.0640 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:23.610 +69:58:22.65
Second-epoch second image center 23:59:21.829 +69:58:08.10
Angular distance between the image centers 0.00477 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.M5zIFd8kV8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.rDEKFMpZQa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits &> /tmp/tmp.nL5r11Iz4q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits &> /tmp/tmp.CEpflBU7Sq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat' -> 'wcsmag.cat'
Read 16658 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0025 to 359.9970 deg, Dec +62.8658 to +75.5048 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0025 to 359.9970 deg, Dec 62.8658 to 75.5048 deg
Loaded 84082 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8746 out of 9568 total matches.
Matched with Tycho-2 9568 out of 16658 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942221
a=0.000000 b=1.000000 c=22.942221
From vast_summary.log: estimated ref. image limiting mag.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.6 pix fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
2.6 pix fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
13.5 mag. fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
13.6 mag. fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.M5zIFd8kV8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1610, passed=16658
Got 16658 stars (including 15034 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 16658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.9470 through 0 to 28.4123, gap 28.4123 to 332.9470
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.9477 through 0 to 28.4145, gap 28.4145 to 332.9477
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16286 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16286 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rDEKFMpZQa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1667, passed=16773
Got 16773 stars (including 15086 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 16773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 333.1738 through 0 to 27.8274, gap 27.8274 to 333.1738
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 338 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 286 matched stars entering correct_measured_positions(), 248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.96"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 281 matched stars entering correct_measured_positions(), 4475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 333.1326 through 0 to 27.8046, gap 27.8046 to 333.1326
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 387 matched stars entering correct_measured_positions(), 4504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.13"
WARNING: Accuracy estimation diagnostic: 386 matched stars entering correct_measured_positions(), 5814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.47"
Excluding outliers - 386 stars left (next iteration limit 309)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nL5r11Iz4q (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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=524, passed=4605
Got 4605 stars (including 4074 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 4605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 332.3124 through 0 to 26.9332, gap 26.9332 to 332.3124
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.1)
Done reading UCAC5 zone files...
Matched 248 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 195 matched stars entering correct_measured_positions(), 130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.95"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 192 matched stars entering correct_measured_positions(), 836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.53"
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 332.3037 through 0 to 26.9099, gap 26.9099 to 332.3037
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.1)
Done reading UCAC5 zone files...
Matched 299 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 261 matched stars entering correct_measured_positions(), 874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.76"
WARNING: Accuracy estimation diagnostic: 261 matched stars entering correct_measured_positions(), 1175 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.30"
Excluding outliers - 261 stars left (next iteration limit 211)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.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.CEpflBU7Sq (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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=529, passed=4905
Got 4905 stars (including 4369 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 4905 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 332.3129 through 0 to 26.9325, gap 26.9325 to 332.3129
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.1)
Done reading UCAC5 zone files...
Matched 255 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 194 matched stars entering correct_measured_positions(), 134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.78"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 186 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.35"
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 332.2978 through 0 to 26.9135, gap 26.9135 to 332.2978
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.1)
Done reading UCAC5 zone files...
Matched 298 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 262 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.82"
WARNING: Accuracy estimation diagnostic: 262 matched stars entering correct_measured_positions(), 1232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.19"
Excluding outliers - 262 stars left (next iteration limit 204)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits'
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21107.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 20822_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 20822_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 20884_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20884_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:01:50.01 +65:46:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.20, MAG_FAINT_SEARCH_LIMIT=10.18)GAIADR2_OUTPUT=# 4.324 2211890191597226368 345.45557550364 +65.77053862218 8.7581 7.8739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20898_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20898_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:00:44.93 +65:34:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.34, MAG_FAINT_SEARCH_LIMIT=10.32)GAIADR2_OUTPUT=# 1.185 2211883628886865024 345.18741216570 +65.57604297636 9.1156 8.7354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20912_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 20912_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 20924_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20924_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:13.23 +65:11:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.59, MAG_FAINT_SEARCH_LIMIT=10.57)GAIADR2_OUTPUT=# 3.164 2208848976795526912 346.05566251963 +65.19962736549 9.4069 9.0491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20937_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20937_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:17.30 +65:07:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.69, MAG_FAINT_SEARCH_LIMIT=10.67)GAIADR2_OUTPUT=# 1.910 2208797883864632064 346.32205356709 +65.13064161695 9.5102 9.3495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20949_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20949_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:59.05 +65:19:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.83, MAG_FAINT_SEARCH_LIMIT=10.81)GAIADR2_OUTPUT=# 0.319 2208897767624763776 346.74611225773 +65.32408346737 9.7033 9.5500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20959_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20959_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:35.87 +65:22:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.93, MAG_FAINT_SEARCH_LIMIT=10.91)GAIADR2_OUTPUT=# 2.912 2208854955389935104 346.15139311643 +65.38040303075 9.6916 9.1772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20965_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 20965_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:02.60 +65:14:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20990_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 20990_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 21043_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 21043_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:03:28.19 +65:39:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)GAIADR2_OUTPUT=# 5.571 2211878990322601216 345.87098493424 +65.66160764183 10.2556 9.7752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21063_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 21063_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 21107_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 21107_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:51:33.87 +68:35:26.3
23:06:51.69 +65:33:41.4
00:12:09.07 +73:45:59.8
23:00:04.34 +65:59:09.6
23:02:17.28 +65:10:48.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:23.610 +69:58:22.65
Angular distance between the image centers 0.0600 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:02.007 +69:59:50.87
Second-epoch image center 23:59:21.829 +69:58:08.10
Angular distance between the image centers 0.0640 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:23.610 +69:58:22.65
Second-epoch second image center 23:59:21.829 +69:58:08.10
Angular distance between the image centers 0.00477 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.6J5gOhklTE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.88nBbpnbAa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits &> /tmp/tmp.BhD352rMw9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits &> /tmp/tmp.piRVCpabw7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat' -> 'wcsmag.cat'
Read 114234 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9997 deg, Dec +62.7863 to +75.5048 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0012 to 359.9997 deg, Dec 62.7863 to 75.5048 deg
Loaded 84921 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 7448 out of 9832 total matches.
Matched with Tycho-2 9832 out of 114234 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779293
a=0.000000 b=1.000000 c=22.779293
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 194 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.1 pix fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
2.2 pix fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
13.8 mag. fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
13.9 mag. fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6J5gOhklTE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=12405, passed=114192
Got 114192 stars (including 101585 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 114192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.6411 through 0 to 28.4717, gap 28.4717 to 332.6411
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.88nBbpnbAa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=12319, passed=113226
Got 113226 stars (including 100709 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 113226 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.7589 through 0 to 27.9073, gap 27.9073 to 332.7589
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 349 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 300 matched stars entering correct_measured_positions(), 256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.18"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 293 matched stars entering correct_measured_positions(), 27938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.7145 through 0 to 27.8794, gap 27.8794 to 332.7145
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 414 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 384 matched stars entering correct_measured_positions(), 27964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.74"
WARNING: Accuracy estimation diagnostic: 384 matched stars entering correct_measured_positions(), 35081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 384 stars left (next iteration limit 322)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BhD352rMw9 (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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1725, passed=38646
Got 38646 stars (including 36856 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 38646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 332.0711 through 0 to 27.0200, gap 27.0200 to 332.0711
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 247 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 195 matched stars entering correct_measured_positions(), 130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.82"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 190 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.28"
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 332.0511 through 0 to 27.0008, gap 27.0008 to 332.0511
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 296 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 258 matched stars entering correct_measured_positions(), 4954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.12"
WARNING: Accuracy estimation diagnostic: 258 matched stars entering correct_measured_positions(), 7664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.56"
Excluding outliers - 258 stars left (next iteration limit 209)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.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.piRVCpabw7 (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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.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_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1831, passed=40561
Got 40561 stars (including 38667 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 40561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 332.0703 through 0 to 27.1569, gap 27.1569 to 332.0703
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 246 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 193 matched stars entering correct_measured_positions(), 129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.14"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 188 matched stars entering correct_measured_positions(), 5170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 332.0574 through 0 to 27.1340, gap 27.1340 to 332.0574
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 294 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 5212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.45"
WARNING: Accuracy estimation diagnostic: 257 matched stars entering correct_measured_positions(), 7721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.87"
Excluding outliers - 257 stars left (next iteration limit 206)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits -region wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-01_20.00sec_-4.90C_LIGHT_0004.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cep-03-Q2b1x1_210426_TTUQ2b1x1_22208_HuvpWmkq/wcs_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005.fits
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out133187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out133074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90961.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 201s
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: 88s
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Considering the candidate 133074_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133074_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133078_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133078_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133079_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133079_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133083_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133083_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133087_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133087_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133088_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133088_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 133089_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133089_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133094_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133094_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133098_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133098_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 133099_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133099_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 133100_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133100_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133101_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133101_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133103_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133103_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133104_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133104_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 133107_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133107_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133108_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133108_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133109_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133109_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 133110_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133110_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133115_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133115_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133116_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133116_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133119_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133119_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133126_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133126_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133127_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133127_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133172_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133172_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:02.24 +65:11:34.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133187_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133187_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:01:49.83 +65:46:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.28, MAG_FAINT_SEARCH_LIMIT=10.26)GAIADR2_OUTPUT=# 3.208 2211890191597226368 345.45557550364 +65.77053862218 8.7581 7.8739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133204_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133204_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:00:44.99 +65:34:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.42, MAG_FAINT_SEARCH_LIMIT=10.40)GAIADR2_OUTPUT=# 0.748 2211883628886865024 345.18741216570 +65.57604297636 9.1156 8.7354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133214_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133214_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:51.65 +65:33:41.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133223_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133223_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:13.03 +65:11:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.66, MAG_FAINT_SEARCH_LIMIT=10.64)GAIADR2_OUTPUT=# 4.291 2208848976795526912 346.05566251963 +65.19962736549 9.4069 9.0491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133230_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133230_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:17.13 +65:07:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.74, MAG_FAINT_SEARCH_LIMIT=10.72)GAIADR2_OUTPUT=# 5.310 2208797883864632064 346.32205356709 +65.13064161695 9.5102 9.3495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133250_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133250_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:58.96 +65:19:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.90, MAG_FAINT_SEARCH_LIMIT=10.88)GAIADR2_OUTPUT=# 0.734 2208897767624763776 346.74611225773 +65.32408346737 9.7033 9.5500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133261_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133261_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:35.72 +65:22:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.01, MAG_FAINT_SEARCH_LIMIT=10.99)GAIADR2_OUTPUT=# 3.855 2208854955389935104 346.15139311643 +65.38040303075 9.6916 9.1772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133266_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133266_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:02.44 +65:14:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133293_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133293_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133338_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133338_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133361_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133361_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:00:03.97 +65:59:08.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133365_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133365_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133410_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133410_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:02:17.09 +65:10:49.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133437_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133437_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133438_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133438_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133463_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133463_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133477_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133477_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133488_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133488_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133501_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133501_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133503_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133503_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133509_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133509_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133518_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133518_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133536_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133536_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133545_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133545_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133547_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133547_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133560_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133560_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133563_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133563_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133589_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133589_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133599_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133599_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133600_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133600_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133639_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133639_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133655_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133655_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133658_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133658_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 133663_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133663_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133698_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133698_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133713_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133713_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133728_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133728_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133731_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133731_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133762_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133762_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133771_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133771_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133773_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133773_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133783_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133783_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133788_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133788_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133811_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133811_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133826_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133826_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133834_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133834_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133902_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133902_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133903_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133903_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 133906_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133906_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133910_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133910_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133917_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 133917_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 133930_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133930_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133943_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133943_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133951_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133951_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 133956_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 133956_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134014_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134014_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 134030_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134030_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134031_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134031_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134066_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134066_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134067_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134067_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134079_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134079_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134132_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134132_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
**** FOUND 23:47:51.26 +67:47:37.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134138_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134138_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134150_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134150_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134155_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134155_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134164_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134164_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134196_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134196_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134275_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134275_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (33.2") between the two second-epoch detections
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Considering the candidate 134283_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134283_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134304_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134304_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134354_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134354_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134374_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134374_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134380_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134380_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134399_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134399_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134400_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134400_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134407_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134407_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 134408_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134408_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 134431_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134431_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 134442_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134442_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134473_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134473_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134480_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134480_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134503_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134503_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134505_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134505_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134532_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134532_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134534_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134534_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 134549_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134549_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134550_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134550_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134551_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134551_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134575_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134575_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134584_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134584_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134589_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134589_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 134590_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134590_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134599_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134599_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 134605_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134605_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134613_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134613_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134622_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134622_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134626_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134626_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 134684_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134684_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134689_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134689_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134704_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134704_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134713_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134713_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134717_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134717_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134727_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134727_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 134730_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134730_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134733_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134733_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134738_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134738_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134748_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134748_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134753_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134753_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 134767_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134767_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 134770_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134770_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134774_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134774_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134784_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134784_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134816_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134816_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134831_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134831_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134834_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134834_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134840_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134840_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134855_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134855_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134888_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134888_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134892_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134892_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134912_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134912_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134934_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134934_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134955_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134955_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134957_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134957_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134965_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134965_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134967_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134967_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134979_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134979_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134991_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134991_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 134993_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 134993_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 134994_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 134994_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 135018_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135018_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135031_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135031_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135037_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135037_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 135067_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135067_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135068_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135068_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135073_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135073_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135099_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135099_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135129_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135129_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135130_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135130_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 135178_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135178_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135208_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135208_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135220_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135220_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135248_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135248_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135260_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135260_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 135286_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135286_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135332_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135332_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135340_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135340_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135360_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135360_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135370_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135370_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 135379_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135379_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135389_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135389_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 135390_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135390_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135423_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135423_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 135440_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135440_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 135468_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135468_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 135507_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135507_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 135534_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135534_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135547_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135547_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135554_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135554_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135559_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135559_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 135572_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135572_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 135587_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 135587_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 135608_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 135608_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 124954_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 124954_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 13668_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 13668_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 85200_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 85200_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 45630_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 45630_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 63520_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
The candidate 63520_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 90961_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 90961_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 31670_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 31670_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
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Considering the candidate 87145_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
Preparing report for the candidate 87145_fd_Cep-03-Q2b1x1_2026-04-05_21-03-46_20.00sec_-5.00C_LIGHT_0005
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 296s
Prepared the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:51:33.87 +68:35:26.3
23:06:51.69 +65:33:41.4
00:12:09.07 +73:45:59.8
23:00:04.34 +65:59:09.6
23:02:17.28 +65:10:48.0
00:45:10.92 +72:45:23.8
23:52:44.11 +67:07:04.9
00:55:43.67 +70:46:36.2
00:15:42.40 +70:48:35.7
00:51:52.60 +65:50:58.4
01:24:23.11 +72:27:05.6
00:26:24.15 +69:06:34.9
22:56:10.09 +67:18:07.4
22:55:35.10 +70:54:30.2
01:06:41.04 +72:08:23.7
23:08:56.80 +65:32:43.0
23:18:47.92 +65:49:40.1
23:35:17.73 +68:52:31.9
23:10:53.12 +65:42:44.5
23:04:45.82 +67:07:53.3
23:15:26.19 +65:47:20.5
01:24:17.31 +72:58:58.7
23:00:38.08 +66:31:35.0
23:09:15.10 +65:13:45.6
23:03:28.04 +65:39:43.2
23:03:36.49 +65:45:06.3
23:00:11.56 +66:03:25.7
23:07:54.16 +65:20:56.7
22:55:31.56 +68:36:53.6
23:06:33.72 +65:29:29.7
23:04:28.63 +65:19:30.5
23:03:04.30 +65:56:43.6
22:59:48.71 +66:21:23.9
23:07:32.01 +65:27:47.7
23:02:04.96 +65:03:02.2
23:03:10.22 +65:42:31.4
23:03:09.53 +65:19:44.7
23:00:48.11 +65:33:54.6
23:02:52.09 +65:50:09.9
23:53:48.16 +65:48:47.8
23:05:18.32 +65:31:39.8
23:05:07.35 +65:30:21.2
23:05:42.31 +65:32:04.9
23:06:58.28 +65:15:07.0
23:06:06.12 +65:27:15.0
23:00:48.36 +65:42:55.6
23:01:07.96 +65:35:48.0
23:03:38.70 +65:16:16.3
23:06:50.18 +65:21:24.6
23:01:30.01 +65:31:21.1
23:03:41.69 +65:58:08.4
23:03:53.89 +65:14:26.0
23:24:33.29 +66:31:16.4
23:05:29.34 +65:09:27.1
23:03:44.06 +65:39:58.5
23:06:18.02 +65:37:35.0
23:03:16.32 +65:15:19.5
23:08:36.76 +65:22:09.5
23:06:35.00 +65:23:25.1
23:11:21.66 +65:18:06.0
23:09:30.90 +65:13:11.2
23:01:07.08 +65:49:04.3
23:39:23.63 +70:51:11.2
23:08:19.52 +65:19:39.6
23:04:27.66 +65:35:50.6
23:03:09.65 +65:48:07.7
23:01:28.09 +65:59:26.4
23:03:44.66 +65:04:47.2
23:10:17.98 +68:50:04.0
23:01:17.37 +65:58:07.1
23:01:51.52 +65:34:34.3
01:15:12.88 +72:49:34.0
23:11:27.09 +67:30:54.1
23:05:20.78 +65:40:27.7
23:02:00.83 +65:09:25.4
23:02:06.40 +65:38:56.9
23:09:07.75 +73:12:52.4
23:02:53.09 +65:02:59.1
23:04:05.06 +65:12:51.2
23:13:58.47 +72:03:57.0
23:04:42.83 +65:30:34.4
00:24:11.62 +71:45:11.0
23:09:57.33 +65:17:01.2
23:03:12.54 +65:26:41.6
01:15:42.20 +72:48:33.1
23:18:11.90 +68:07:28.7
23:02:41.90 +65:30:14.8
23:55:31.64 +66:52:04.4
00:09:52.66 +72:50:15.9
23:01:38.66 +65:33:26.2
23:04:31.84 +65:37:15.0
23:08:43.83 +65:18:58.0
23:04:54.79 +68:25:36.6
23:02:36.49 +65:20:20.9
00:36:10.56 +72:49:47.2
23:00:07.42 +65:40:04.5
23:06:13.80 +65:26:17.9
23:03:19.38 +65:48:13.4
00:00:21.08 +70:53:46.6
23:06:21.18 +65:16:38.1
23:05:17.10 +65:19:06.5
23:20:04.61 +73:52:01.2
23:04:18.76 +65:31:37.4
23:02:51.68 +65:54:29.6
22:50:09.73 +69:55:54.0
23:01:38.13 +65:29:41.8
23:05:13.93 +65:36:51.3
23:37:08.25 +68:44:29.2
23:01:37.71 +65:32:08.6
23:11:19.63 +65:19:39.8
23:07:45.95 +65:22:48.0
23:02:44.15 +65:39:19.4
00:10:49.22 +69:38:01.1
00:03:32.06 +69:18:01.3
23:00:30.65 +66:04:50.5
00:36:58.95 +71:06:57.4
23:05:26.15 +65:33:46.4
23:02:39.87 +65:28:34.5
23:05:45.93 +65:19:14.1
23:27:11.51 +65:36:14.4
23:36:31.64 +67:50:16.7
23:27:17.68 +70:16:08.9
23:04:13.12 +66:15:56.2
23:01:27.14 +65:38:20.7
00:21:43.26 +72:13:54.4
23:08:42.91 +65:27:33.8
23:03:03.92 +65:51:47.5
23:03:50.91 +65:53:51.7
23:56:48.79 +72:46:02.2
23:55:13.29 +72:44:35.3
23:01:27.96 +65:23:30.9
23:39:16.06 +70:44:56.6
00:31:51.42 +69:56:50.3
23:22:29.79 +71:46:49.1
23:06:23.35 +65:44:36.2
00:14:02.73 +72:03:23.2
00:36:49.52 +71:09:00.6
23:38:49.43 +73:57:46.4
23:51:34.45 +72:42:02.0
23:14:29.15 +70:33:46.8
00:27:50.91 +68:14:03.8
00:01:36.29 +67:23:46.7
00:12:10.74 +73:45:57.3
01:01:57.06 +70:59:43.4
00:33:38.91 +70:41:55.1
23:02:29.09 +66:07:08.9
23:07:59.20 +67:50:12.1
23:00:11.95 +66:36:21.4
########### Completed Cep-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:51:33.87 +68:35:26.3
23:06:51.69 +65:33:41.4
00:12:09.07 +73:45:59.8
23:00:04.34 +65:59:09.6
23:02:17.28 +65:10:48.0
00:45:10.92 +72:45:23.8
23:52:44.11 +67:07:04.9
00:55:43.67 +70:46:36.2
00:15:42.40 +70:48:35.7
00:51:52.60 +65:50:58.4
01:24:23.11 +72:27:05.6
00:26:24.15 +69:06:34.9
22:56:10.09 +67:18:07.4
22:55:35.10 +70:54:30.2
01:06:41.04 +72:08:23.7
23:08:56.80 +65:32:43.0
23:18:47.92 +65:49:40.1
23:35:17.73 +68:52:31.9
23:10:53.12 +65:42:44.5
23:04:45.82 +67:07:53.3
23:15:26.19 +65:47:20.5
01:24:17.31 +72:58:58.7
23:00:38.08 +66:31:35.0
23:09:15.10 +65:13:45.6
23:03:28.04 +65:39:43.2
23:03:36.49 +65:45:06.3
23:00:11.56 +66:03:25.7
23:07:54.16 +65:20:56.7
22:55:31.56 +68:36:53.6
23:06:33.72 +65:29:29.7
23:04:28.63 +65:19:30.5
23:03:04.30 +65:56:43.6
22:59:48.71 +66:21:23.9
23:07:32.01 +65:27:47.7
23:02:04.96 +65:03:02.2
23:03:10.22 +65:42:31.4
23:03:09.53 +65:19:44.7
23:00:48.11 +65:33:54.6
23:02:52.09 +65:50:09.9
23:53:48.16 +65:48:47.8
23:05:18.32 +65:31:39.8
23:05:07.35 +65:30:21.2
23:05:42.31 +65:32:04.9
23:06:58.28 +65:15:07.0
23:06:06.12 +65:27:15.0
23:00:48.36 +65:42:55.6
23:01:07.96 +65:35:48.0
23:03:38.70 +65:16:16.3
23:06:50.18 +65:21:24.6
23:01:30.01 +65:31:21.1
23:03:41.69 +65:58:08.4
23:03:53.89 +65:14:26.0
23:24:33.29 +66:31:16.4
23:05:29.34 +65:09:27.1
23:03:44.06 +65:39:58.5
23:06:18.02 +65:37:35.0
23:03:16.32 +65:15:19.5
23:08:36.76 +65:22:09.5
23:06:35.00 +65:23:25.1
23:11:21.66 +65:18:06.0
23:09:30.90 +65:13:11.2
23:01:07.08 +65:49:04.3
23:39:23.63 +70:51:11.2
23:08:19.52 +65:19:39.6
23:04:27.66 +65:35:50.6
23:03:09.65 +65:48:07.7
23:01:28.09 +65:59:26.4
23:03:44.66 +65:04:47.2
23:10:17.98 +68:50:04.0
23:01:17.37 +65:58:07.1
23:01:51.52 +65:34:34.3
01:15:12.88 +72:49:34.0
23:11:27.09 +67:30:54.1
23:05:20.78 +65:40:27.7
23:02:00.83 +65:09:25.4
23:02:06.40 +65:38:56.9
23:09:07.75 +73:12:52.4
23:02:53.09 +65:02:59.1
23:04:05.06 +65:12:51.2
23:13:58.47 +72:03:57.0
23:04:42.83 +65:30:34.4
00:24:11.62 +71:45:11.0
23:09:57.33 +65:17:01.2
23:03:12.54 +65:26:41.6
01:15:42.20 +72:48:33.1
23:18:11.90 +68:07:28.7
23:02:41.90 +65:30:14.8
23:55:31.64 +66:52:04.4
00:09:52.66 +72:50:15.9
23:01:38.66 +65:33:26.2
23:04:31.84 +65:37:15.0
23:08:43.83 +65:18:58.0
23:04:54.79 +68:25:36.6
23:02:36.49 +65:20:20.9
00:36:10.56 +72:49:47.2
23:00:07.42 +65:40:04.5
23:06:13.80 +65:26:17.9
23:03:19.38 +65:48:13.4
00:00:21.08 +70:53:46.6
23:06:21.18 +65:16:38.1
23:05:17.10 +65:19:06.5
23:20:04.61 +73:52:01.2
23:04:18.76 +65:31:37.4
23:02:51.68 +65:54:29.6
22:50:09.73 +69:55:54.0
23:01:38.13 +65:29:41.8
23:05:13.93 +65:36:51.3
23:37:08.25 +68:44:29.2
23:01:37.71 +65:32:08.6
23:11:19.63 +65:19:39.8
23:07:45.95 +65:22:48.0
23:02:44.15 +65:39:19.4
00:10:49.22 +69:38:01.1
00:03:32.06 +69:18:01.3
23:00:30.65 +66:04:50.5
00:36:58.95 +71:06:57.4
23:05:26.15 +65:33:46.4
23:02:39.87 +65:28:34.5
23:05:45.93 +65:19:14.1
23:27:11.51 +65:36:14.4
23:36:31.64 +67:50:16.7
23:27:17.68 +70:16:08.9
23:04:13.12 +66:15:56.2
23:01:27.14 +65:38:20.7
00:21:43.26 +72:13:54.4
23:08:42.91 +65:27:33.8
23:03:03.92 +65:51:47.5
23:03:50.91 +65:53:51.7
23:56:48.79 +72:46:02.2
23:55:13.29 +72:44:35.3
23:01:27.96 +65:23:30.9
23:39:16.06 +70:44:56.6
00:31:51.42 +69:56:50.3
23:22:29.79 +71:46:49.1
23:06:23.35 +65:44:36.2
00:14:02.73 +72:03:23.2
00:36:49.52 +71:09:00.6
23:38:49.43 +73:57:46.4
23:51:34.45 +72:42:02.0
23:14:29.15 +70:33:46.8
00:27:50.91 +68:14:03.8
00:01:36.29 +67:23:46.7
00:12:10.74 +73:45:57.3
23:02:29.09 +66:07:08.9
00:33:38.91 +70:41:55.1
23:00:11.95 +66:36:21.4
01:01:57.06 +70:59:43.4
23:07:59.20 +67:50:12.1
###################################################################################
00:51:33.87 +68:35:26.3 -- not an asteroid (will add it to exclusion list)
23:06:51.69 +65:33:41.4 -- not an asteroid (will add it to exclusion list)
00:12:09.07 +73:45:59.8 -- not an asteroid (will add it to exclusion list)
23:00:04.34 +65:59:09.6 -- not an asteroid (will add it to exclusion list)
23:02:17.28 +65:10:48.0 -- not an asteroid (will add it to exclusion list)
00:45:10.92 +72:45:23.8 -- not an asteroid (will add it to exclusion list)
23:52:44.11 +67:07:04.9 -- not an asteroid (will add it to exclusion list)
00:55:43.67 +70:46:36.2 -- not an asteroid (will add it to exclusion list)
00:15:42.40 +70:48:35.7 -- not an asteroid (will add it to exclusion list)
00:51:52.60 +65:50:58.4 -- not an asteroid (will add it to exclusion list)
01:24:23.11 +72:27:05.6 -- not an asteroid (will add it to exclusion list)
00:26:24.15 +69:06:34.9 -- not an asteroid (will add it to exclusion list)
22:56:10.09 +67:18:07.4 -- not an asteroid (will add it to exclusion list)
22:55:35.10 +70:54:30.2 -- not an asteroid (will add it to exclusion list)
01:06:41.04 +72:08:23.7 -- not an asteroid (will add it to exclusion list)
23:08:56.80 +65:32:43.0 -- not an asteroid (will add it to exclusion list)
23:18:47.92 +65:49:40.1 -- not an asteroid (will add it to exclusion list)
23:35:17.73 +68:52:31.9 -- not an asteroid (will add it to exclusion list)
23:10:53.12 +65:42:44.5 -- not an asteroid (will add it to exclusion list)
23:04:45.82 +67:07:53.3 -- not an asteroid (will add it to exclusion list)
23:15:26.19 +65:47:20.5 -- not an asteroid (will add it to exclusion list)
01:24:17.31 +72:58:58.7 -- not an asteroid (will add it to exclusion list)
23:00:38.08 +66:31:35.0 -- not an asteroid (will add it to exclusion list)
23:09:15.10 +65:13:45.6 -- not an asteroid (will add it to exclusion list)
23:03:28.04 +65:39:43.2 -- not an asteroid (will add it to exclusion list)
23:03:36.49 +65:45:06.3 -- not an asteroid (will add it to exclusion list)
23:00:11.56 +66:03:25.7 -- not an asteroid (will add it to exclusion list)
23:07:54.16 +65:20:56.7 -- not an asteroid (will add it to exclusion list)
22:55:31.56 +68:36:53.6 -- not an asteroid (will add it to exclusion list)
23:06:33.72 +65:29:29.7 -- not an asteroid (will add it to exclusion list)
23:04:28.63 +65:19:30.5 -- not an asteroid (will add it to exclusion list)
23:03:04.30 +65:56:43.6 -- not an asteroid (will add it to exclusion list)
22:59:48.71 +66:21:23.9 -- not an asteroid (will add it to exclusion list)
23:07:32.01 +65:27:47.7 -- not an asteroid (will add it to exclusion list)
23:02:04.96 +65:03:02.2 -- not an asteroid (will add it to exclusion list)
23:03:10.22 +65:42:31.4 -- not an asteroid (will add it to exclusion list)
23:03:09.53 +65:19:44.7 -- not an asteroid (will add it to exclusion list)
23:00:48.11 +65:33:54.6 -- not an asteroid (will add it to exclusion list)
23:02:52.09 +65:50:09.9 -- not an asteroid (will add it to exclusion list)
23:53:48.16 +65:48:47.8 -- not an asteroid (will add it to exclusion list)
23:05:18.32 +65:31:39.8 -- not an asteroid (will add it to exclusion list)
23:05:07.35 +65:30:21.2 -- not an asteroid (will add it to exclusion list)
23:05:42.31 +65:32:04.9 -- not an asteroid (will add it to exclusion list)
23:06:58.28 +65:15:07.0 -- not an asteroid (will add it to exclusion list)
23:06:06.12 +65:27:15.0 -- not an asteroid (will add it to exclusion list)
23:00:48.36 +65:42:55.6 -- not an asteroid (will add it to exclusion list)
23:01:07.96 +65:35:48.0 -- not an asteroid (will add it to exclusion list)
23:03:38.70 +65:16:16.3 -- not an asteroid (will add it to exclusion list)
23:06:50.18 +65:21:24.6 -- not an asteroid (will add it to exclusion list)
23:01:30.01 +65:31:21.1 -- not an asteroid (will add it to exclusion list)
23:03:41.69 +65:58:08.4 -- not an asteroid (will add it to exclusion list)
23:03:53.89 +65:14:26.0 -- not an asteroid (will add it to exclusion list)
23:24:33.29 +66:31:16.4 -- not an asteroid (will add it to exclusion list)
23:05:29.34 +65:09:27.1 -- not an asteroid (will add it to exclusion list)
23:03:44.06 +65:39:58.5 -- not an asteroid (will add it to exclusion list)
23:06:18.02 +65:37:35.0 -- not an asteroid (will add it to exclusion list)
23:03:16.32 +65:15:19.5 -- not an asteroid (will add it to exclusion list)
23:08:36.76 +65:22:09.5 -- not an asteroid (will add it to exclusion list)
23:06:35.00 +65:23:25.1 -- not an asteroid (will add it to exclusion list)
23:11:21.66 +65:18:06.0 -- not an asteroid (will add it to exclusion list)
23:09:30.90 +65:13:11.2 -- not an asteroid (will add it to exclusion list)
23:01:07.08 +65:49:04.3 -- not an asteroid (will add it to exclusion list)
23:39:23.63 +70:51:11.2 -- not an asteroid (will add it to exclusion list)
23:08:19.52 +65:19:39.6 -- not an asteroid (will add it to exclusion list)
23:04:27.66 +65:35:50.6 -- not an asteroid (will add it to exclusion list)
23:03:09.65 +65:48:07.7 -- not an asteroid (will add it to exclusion list)
23:01:28.09 +65:59:26.4 -- not an asteroid (will add it to exclusion list)
23:03:44.66 +65:04:47.2 -- not an asteroid (will add it to exclusion list)
23:10:17.98 +68:50:04.0 -- not an asteroid (will add it to exclusion list)
23:01:17.37 +65:58:07.1 -- not an asteroid (will add it to exclusion list)
23:01:51.52 +65:34:34.3 -- not an asteroid (will add it to exclusion list)
01:15:12.88 +72:49:34.0 -- not an asteroid (will add it to exclusion list)
23:11:27.09 +67:30:54.1 -- not an asteroid (will add it to exclusion list)
23:05:20.78 +65:40:27.7 -- not an asteroid (will add it to exclusion list)
23:02:00.83 +65:09:25.4 -- not an asteroid (will add it to exclusion list)
23:02:06.40 +65:38:56.9 -- not an asteroid (will add it to exclusion list)
23:09:07.75 +73:12:52.4 -- not an asteroid (will add it to exclusion list)
23:02:53.09 +65:02:59.1 -- not an asteroid (will add it to exclusion list)
23:04:05.06 +65:12:51.2 -- not an asteroid (will add it to exclusion list)
23:13:58.47 +72:03:57.0 -- not an asteroid (will add it to exclusion list)
23:04:42.83 +65:30:34.4 -- not an asteroid (will add it to exclusion list)
00:24:11.62 +71:45:11.0 -- not an asteroid (will add it to exclusion list)
23:09:57.33 +65:17:01.2 -- not an asteroid (will add it to exclusion list)
23:03:12.54 +65:26:41.6 -- not an asteroid (will add it to exclusion list)
01:15:42.20 +72:48:33.1 -- not an asteroid (will add it to exclusion list)
23:18:11.90 +68:07:28.7 -- not an asteroid (will add it to exclusion list)
23:02:41.90 +65:30:14.8 -- not an asteroid (will add it to exclusion list)
23:55:31.64 +66:52:04.4 -- not an asteroid (will add it to exclusion list)
00:09:52.66 +72:50:15.9 -- not an asteroid (will add it to exclusion list)
23:01:38.66 +65:33:26.2 -- not an asteroid (will add it to exclusion list)
23:04:31.84 +65:37:15.0 -- not an asteroid (will add it to exclusion list)
23:08:43.83 +65:18:58.0 -- not an asteroid (will add it to exclusion list)
23:04:54.79 +68:25:36.6 -- not an asteroid (will add it to exclusion list)
23:02:36.49 +65:20:20.9 -- not an asteroid (will add it to exclusion list)
00:36:10.56 +72:49:47.2 -- not an asteroid (will add it to exclusion list)
23:00:07.42 +65:40:04.5 -- not an asteroid (will add it to exclusion list)
23:06:13.80 +65:26:17.9 -- not an asteroid (will add it to exclusion list)
23:03:19.38 +65:48:13.4 -- not an asteroid (will add it to exclusion list)
00:00:21.08 +70:53:46.6 -- not an asteroid (will add it to exclusion list)
23:06:21.18 +65:16:38.1 -- not an asteroid (will add it to exclusion list)
23:05:17.10 +65:19:06.5 -- not an asteroid (will add it to exclusion list)
23:20:04.61 +73:52:01.2 -- not an asteroid (will add it to exclusion list)
23:04:18.76 +65:31:37.4 -- not an asteroid (will add it to exclusion list)
23:02:51.68 +65:54:29.6 -- not an asteroid (will add it to exclusion list)
22:50:09.73 +69:55:54.0 -- not an asteroid (will add it to exclusion list)
23:01:38.13 +65:29:41.8 -- not an asteroid (will add it to exclusion list)
23:05:13.93 +65:36:51.3 -- not an asteroid (will add it to exclusion list)
23:37:08.25 +68:44:29.2 -- not an asteroid (will add it to exclusion list)
23:01:37.71 +65:32:08.6 -- not an asteroid (will add it to exclusion list)
23:11:19.63 +65:19:39.8 -- not an asteroid (will add it to exclusion list)
23:07:45.95 +65:22:48.0 -- not an asteroid (will add it to exclusion list)
23:02:44.15 +65:39:19.4 -- not an asteroid (will add it to exclusion list)
00:10:49.22 +69:38:01.1 -- not an asteroid (will add it to exclusion list)
00:03:32.06 +69:18:01.3 -- not an asteroid (will add it to exclusion list)
23:00:30.65 +66:04:50.5 -- not an asteroid (will add it to exclusion list)
00:36:58.95 +71:06:57.4 -- not an asteroid (will add it to exclusion list)
23:05:26.15 +65:33:46.4 -- not an asteroid (will add it to exclusion list)
23:02:39.87 +65:28:34.5 -- not an asteroid (will add it to exclusion list)
23:05:45.93 +65:19:14.1 -- not an asteroid (will add it to exclusion list)
23:27:11.51 +65:36:14.4 -- not an asteroid (will add it to exclusion list)
23:36:31.64 +67:50:16.7 -- not an asteroid (will add it to exclusion list)
23:27:17.68 +70:16:08.9 -- not an asteroid (will add it to exclusion list)
23:04:13.12 +66:15:56.2 -- not an asteroid (will add it to exclusion list)
23:01:27.14 +65:38:20.7 -- not an asteroid (will add it to exclusion list)
00:21:43.26 +72:13:54.4 -- not an asteroid (will add it to exclusion list)
23:08:42.91 +65:27:33.8 -- not an asteroid (will add it to exclusion list)
23:03:03.92 +65:51:47.5 -- not an asteroid (will add it to exclusion list)
23:03:50.91 +65:53:51.7 -- not an asteroid (will add it to exclusion list)
23:56:48.79 +72:46:02.2 -- not an asteroid (will add it to exclusion list)
23:55:13.29 +72:44:35.3 -- not an asteroid (will add it to exclusion list)
23:01:27.96 +65:23:30.9 -- not an asteroid (will add it to exclusion list)
23:39:16.06 +70:44:56.6 -- not an asteroid (will add it to exclusion list)
00:31:51.42 +69:56:50.3 -- not an asteroid (will add it to exclusion list)
23:22:29.79 +71:46:49.1 -- not an asteroid (will add it to exclusion list)
23:06:23.35 +65:44:36.2 -- not an asteroid (will add it to exclusion list)
00:14:02.73 +72:03:23.2 -- not an asteroid (will add it to exclusion list)
00:36:49.52 +71:09:00.6 -- not an asteroid (will add it to exclusion list)
23:38:49.43 +73:57:46.4 -- not an asteroid (will add it to exclusion list)
23:51:34.45 +72:42:02.0 -- not an asteroid (will add it to exclusion list)
23:14:29.15 +70:33:46.8 -- not an asteroid (will add it to exclusion list)
00:27:50.91 +68:14:03.8 -- not an asteroid (will add it to exclusion list)
00:01:36.29 +67:23:46.7 -- not an asteroid (will add it to exclusion list)
00:12:10.74 +73:45:57.3 -- not an asteroid (will add it to exclusion list)
23:02:29.09 +66:07:08.9 -- not an asteroid (will add it to exclusion list)
00:33:38.91 +70:41:55.1 -- not an asteroid (will add it to exclusion list)
23:00:11.95 +66:36:21.4 -- not an asteroid (will add it to exclusion list)
01:01:57.06 +70:59:43.4 -- not an asteroid (will add it to exclusion list)
23:07:59.20 +67:50:12.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:21.08 +70:53:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:36.29 +67:23:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:32.06 +69:18:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:52.66 +72:50:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:49.22 +69:38:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:09.07 +73:45:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:10.74 +73:45:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:02.73 +72:03:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:42.40 +70:48:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:43.26 +72:13:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:11.62 +71:45:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:24.15 +69:06:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:50.91 +68:14:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:51.42 +69:56:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:38.91 +70:41:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:10.56 +72:49:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:49.52 +71:09:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:58.95 +71:06:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:10.92 +72:45:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:33.87 +68:35:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:52.60 +65:50:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:43.67 +70:46:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:57.06 +70:59:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:41.04 +72:08:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:12.88 +72:49:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:42.20 +72:48:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:17.31 +72:58:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:23.11 +72:27:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:50:09.73 +69:55:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:55:31.56 +68:36:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:55:35.10 +70:54:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:56:10.09 +67:18:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:48.71 +66:21:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:04.34 +65:59:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:07.42 +65:40:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:11.56 +66:03:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:11.95 +66:36:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:30.65 +66:04:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:38.08 +66:31:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:48.11 +65:33:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:48.36 +65:42:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:07.08 +65:49:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:07.96 +65:35:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:17.37 +65:58:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:27.14 +65:38:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:27.96 +65:23:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:28.09 +65:59:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:30.01 +65:31:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:37.71 +65:32:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:38.13 +65:29:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:38.66 +65:33:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:51.52 +65:34:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:00.83 +65:09:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:04.96 +65:03:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:06.40 +65:38:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:17.28 +65:10:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:29.09 +66:07:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:36.49 +65:20:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:39.87 +65:28:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:41.90 +65:30:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:44.15 +65:39:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:51.68 +65:54:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:52.09 +65:50:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:53.09 +65:02:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:03.92 +65:51:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:04.30 +65:56:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:09.53 +65:19:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:09.65 +65:48:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:10.22 +65:42:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:12.54 +65:26:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:16.32 +65:15:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:19.38 +65:48:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:28.04 +65:39:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:36.49 +65:45:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:38.70 +65:16:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:41.69 +65:58:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:44.06 +65:39:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:44.66 +65:04:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:50.91 +65:53:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:53.89 +65:14:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:05.06 +65:12:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:13.12 +66:15:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:18.76 +65:31:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:27.66 +65:35:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:28.63 +65:19:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:31.84 +65:37:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:42.83 +65:30:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:45.82 +67:07:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:54.79 +68:25:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:07.35 +65:30:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:13.93 +65:36:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:17.10 +65:19:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:18.32 +65:31:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:20.78 +65:40:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:26.15 +65:33:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:29.34 +65:09:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:42.31 +65:32:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:45.93 +65:19:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:06.12 +65:27:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:13.80 +65:26:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:18.02 +65:37:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:21.18 +65:16:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:23.35 +65:44:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:33.72 +65:29:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:35.00 +65:23:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:50.18 +65:21:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:51.69 +65:33:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:58.28 +65:15:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:32.01 +65:27:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:45.95 +65:22:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:54.16 +65:20:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:59.20 +67:50:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:19.52 +65:19:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:36.76 +65:22:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:42.91 +65:27:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:43.83 +65:18:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:56.80 +65:32:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:07.75 +73:12:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:15.10 +65:13:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:30.90 +65:13:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:57.33 +65:17:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:17.98 +68:50:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:53.12 +65:42:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:19.63 +65:19:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:21.66 +65:18:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:27.09 +67:30:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:58.47 +72:03:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:29.15 +70:33:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:26.19 +65:47:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:11.90 +68:07:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:47.92 +65:49:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:04.61 +73:52:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:29.79 +71:46:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:33.29 +66:31:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:11.51 +65:36:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:17.68 +70:16:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:17.73 +68:52:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:31.64 +67:50:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:08.25 +68:44:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:49.43 +73:57:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:16.06 +70:44:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:23.63 +70:51:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:34.45 +72:42:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:44.11 +67:07:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:48.16 +65:48:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:13.29 +72:44:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:31.64 +66:52:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:48.79 +72:46:02.2 -- 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)
00:00:21.08 +70:53:46.6 -- not a known variable star
00:01:36.29 +67:23:46.7 -- not a known variable star
00:03:32.06 +69:18:01.3 -- not a known variable star
00:09:52.66 +72:50:15.9 -- not a known variable star
00:10:49.22 +69:38:01.1 -- not a known variable star
00:12:09.07 +73:45:59.8 -- not a known variable star
00:12:10.74 +73:45:57.3 -- not a known variable star
00:14:02.73 +72:03:23.2 -- not a known variable star
00:15:42.40 +70:48:35.7 -- not a known variable star
00:21:43.26 +72:13:54.4 -- not a known variable star
00:24:11.62 +71:45:11.0 -- not a known variable star
00:26:24.15 +69:06:34.9 -- not a known variable star
00:27:50.91 +68:14:03.8 -- not a known variable star
00:31:51.42 +69:56:50.3 -- not a known variable star
00:33:38.91 +70:41:55.1 -- not a known variable star
00:36:10.56 +72:49:47.2 -- not a known variable star
00:36:49.52 +71:09:00.6 -- not a known variable star
00:36:58.95 +71:06:57.4 -- not a known variable star
00:45:10.92 +72:45:23.8 -- not a known variable star
00:51:33.87 +68:35:26.3 -- not a known variable star
00:51:52.60 +65:50:58.4 -- not a known variable star
00:55:43.67 +70:46:36.2 -- not a known variable star
01:01:57.06 +70:59:43.4 -- not a known variable star
01:06:41.04 +72:08:23.7 -- not a known variable star
01:15:12.88 +72:49:34.0 -- not a known variable star
01:15:42.20 +72:48:33.1 -- not a known variable star
01:24:17.31 +72:58:58.7 -- not a known variable star
01:24:23.11 +72:27:05.6 -- not a known variable star
22:50:09.73 +69:55:54.0 -- not a known variable star
22:55:31.56 +68:36:53.6 -- not a known variable star
22:55:35.10 +70:54:30.2 -- not a known variable star
22:56:10.09 +67:18:07.4 -- not a known variable star
22:59:48.71 +66:21:23.9 -- a known variable star
23:00:04.34 +65:59:09.6 -- not a known variable star
23:00:07.42 +65:40:04.5 -- not a known variable star
23:00:11.56 +66:03:25.7 -- not a known variable star
23:00:11.95 +66:36:21.4 -- a known variable star
23:00:30.65 +66:04:50.5 -- not a known variable star
23:00:38.08 +66:31:35.0 -- not a known variable star
23:00:48.11 +65:33:54.6 -- not a known variable star
23:00:48.36 +65:42:55.6 -- not a known variable star
23:01:07.08 +65:49:04.3 -- not a known variable star
23:01:07.96 +65:35:48.0 -- not a known variable star
23:01:17.37 +65:58:07.1 -- not a known variable star
23:01:27.14 +65:38:20.7 -- not a known variable star
23:01:27.96 +65:23:30.9 -- not a known variable star
23:01:28.09 +65:59:26.4 -- not a known variable star
23:01:30.01 +65:31:21.1 -- not a known variable star
23:01:37.71 +65:32:08.6 -- not a known variable star
23:01:38.13 +65:29:41.8 -- not a known variable star
23:01:38.66 +65:33:26.2 -- not a known variable star
23:01:51.52 +65:34:34.3 -- not a known variable star
23:02:00.83 +65:09:25.4 -- not a known variable star
23:02:04.96 +65:03:02.2 -- not a known variable star
23:02:06.40 +65:38:56.9 -- not a known variable star
23:02:17.28 +65:10:48.0 -- not a known variable star
23:02:29.09 +66:07:08.9 -- not a known variable star
23:02:36.49 +65:20:20.9 -- not a known variable star
23:02:39.87 +65:28:34.5 -- not a known variable star
23:02:41.90 +65:30:14.8 -- not a known variable star
23:02:44.15 +65:39:19.4 -- not a known variable star
23:02:51.68 +65:54:29.6 -- not a known variable star
23:02:52.09 +65:50:09.9 -- not a known variable star
23:02:53.09 +65:02:59.1 -- not a known variable star
23:03:03.92 +65:51:47.5 -- not a known variable star
23:03:04.30 +65:56:43.6 -- not a known variable star
23:03:09.53 +65:19:44.7 -- not a known variable star
23:03:09.65 +65:48:07.7 -- not a known variable star
23:03:10.22 +65:42:31.4 -- not a known variable star
23:03:12.54 +65:26:41.6 -- not a known variable star
23:03:16.32 +65:15:19.5 -- not a known variable star
23:03:19.38 +65:48:13.4 -- not a known variable star
23:03:28.04 +65:39:43.2 -- not a known variable star
23:03:36.49 +65:45:06.3 -- not a known variable star
23:03:38.70 +65:16:16.3 -- not a known variable star
23:03:41.69 +65:58:08.4 -- not a known variable star
23:03:44.06 +65:39:58.5 -- not a known variable star
23:03:44.66 +65:04:47.2 -- not a known variable star
23:03:50.91 +65:53:51.7 -- not a known variable star
23:03:53.89 +65:14:26.0 -- not a known variable star
23:04:05.06 +65:12:51.2 -- not a known variable star
23:04:13.12 +66:15:56.2 -- not a known variable star
23:04:18.76 +65:31:37.4 -- not a known variable star
23:04:27.66 +65:35:50.6 -- not a known variable star
23:04:28.63 +65:19:30.5 -- not a known variable star
23:04:31.84 +65:37:15.0 -- not a known variable star
23:04:42.83 +65:30:34.4 -- not a known variable star
23:04:45.82 +67:07:53.3 -- not a known variable star
23:04:54.79 +68:25:36.6 -- not a known variable star
23:05:07.35 +65:30:21.2 -- not a known variable star
23:05:13.93 +65:36:51.3 -- not a known variable star
23:05:17.10 +65:19:06.5 -- not a known variable star
23:05:18.32 +65:31:39.8 -- not a known variable star
23:05:20.78 +65:40:27.7 -- not a known variable star
23:05:26.15 +65:33:46.4 -- not a known variable star
23:05:29.34 +65:09:27.1 -- not a known variable star
23:05:42.31 +65:32:04.9 -- not a known variable star
23:05:45.93 +65:19:14.1 -- not a known variable star
23:06:06.12 +65:27:15.0 -- not a known variable star
23:06:13.80 +65:26:17.9 -- not a known variable star
23:06:18.02 +65:37:35.0 -- a known variable star
23:06:21.18 +65:16:38.1 -- not a known variable star
23:06:23.35 +65:44:36.2 -- not a known variable star
23:06:33.72 +65:29:29.7 -- a known variable star
23:06:35.00 +65:23:25.1 -- not a known variable star
23:06:50.18 +65:21:24.6 -- not a known variable star
23:06:51.69 +65:33:41.4 -- not a known variable star
23:06:58.28 +65:15:07.0 -- not a known variable star
23:07:32.01 +65:27:47.7 -- not a known variable star
23:07:45.95 +65:22:48.0 -- not a known variable star
23:07:54.16 +65:20:56.7 -- a known variable star
23:07:59.20 +67:50:12.1 -- a known variable star
23:08:19.52 +65:19:39.6 -- not a known variable star
23:08:36.76 +65:22:09.5 -- not a known variable star
23:08:42.91 +65:27:33.8 -- not a known variable star
23:08:43.83 +65:18:58.0 -- not a known variable star
23:08:56.80 +65:32:43.0 -- a known variable star
23:09:07.75 +73:12:52.4 -- not a known variable star
23:09:15.10 +65:13:45.6 -- not a known variable star
23:09:30.90 +65:13:11.2 -- not a known variable star
23:09:57.33 +65:17:01.2 -- not a known variable star
23:10:17.98 +68:50:04.0 -- not a known variable star
23:10:53.12 +65:42:44.5 -- not a known variable star
23:11:19.63 +65:19:39.8 -- not a known variable star
23:11:21.66 +65:18:06.0 -- not a known variable star
23:11:27.09 +67:30:54.1 -- not a known variable star
23:13:58.47 +72:03:57.0 -- not a known variable star
23:14:29.15 +70:33:46.8 -- not a known variable star
23:15:26.19 +65:47:20.5 -- not a known variable star
23:18:11.90 +68:07:28.7 -- not a known variable star
23:18:47.92 +65:49:40.1 -- not a known variable star
23:20:04.61 +73:52:01.2 -- not a known variable star
23:22:29.79 +71:46:49.1 -- not a known variable star
23:24:33.29 +66:31:16.4 -- not a known variable star
23:27:11.51 +65:36:14.4 -- not a known variable star
23:27:17.68 +70:16:08.9 -- not a known variable star
23:35:17.73 +68:52:31.9 -- not a known variable star
23:36:31.64 +67:50:16.7 -- not a known variable star
23:37:08.25 +68:44:29.2 -- not a known variable star
23:38:49.43 +73:57:46.4 -- not a known variable star
23:39:16.06 +70:44:56.6 -- not a known variable star
23:39:23.63 +70:51:11.2 -- not a known variable star
23:51:34.45 +72:42:02.0 -- not a known variable star
23:52:44.11 +67:07:04.9 -- a known variable star
23:53:48.16 +65:48:47.8 -- not a known variable star
23:55:13.29 +72:44:35.3 -- not a known variable star
23:55:31.64 +66:52:04.4 -- not a known variable star
23:56:48.79 +72:46:02.2 -- not a known variable star
Found 140 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
148 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 148 (excluding asteroids and hot pixels, 140 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.58555345 -observatory V36
23:19:57.32 -06:27:38.1 Mercury (0.3mag)
02:20:59.31 +13:48:12.1 Venus (-3.9mag)
23:49:35.79 -02:14:38.0 Mars (1.2mag)
07:08:40.07 +22:52:30.3 Jupiter (-2.2mag)
00:24:42.70 +00:20:54.7 Saturn (0.9mag)
03:45:42.13 +19:41:01.6 Uranus (5.8mag)
00:09:30.89 -00:23:46.0 Neptune (7.8mag)
20:33:13.75 -22:52:29.6 Pluto (14.5mag)
15:53:17.81 -25:37:44.4 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 5 21:06 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.58555345:
07:08:46.32 +22:52:16.1 Io (5.7mag)
07:08:52.97 +22:52:04.0 Europa (5.8mag)
07:08:32.60 +22:52:52.0 Ganymede (5.3mag)
07:08:11.23 +22:53:19.7 Callisto (6.5mag)
07:12:23.22 +22:45:03.9 Himalia (15.3mag)
07:08:35.94 +22:52:38.0 Thebe (16.2mag)
07:12:20.75 +23:13:48.5 Elara (17.2mag)
07:06:52.46 +23:37:42.2 Pasiphae (17.3mag)
07:17:12.00 +22:49:25.6 Carme (18.4mag)
00:24:37.00 +00:20:56.8 Titan (8.8mag)
00:24:39.75 +00:21:09.7 Rhea (10.1mag)
00:24:43.52 +00:22:29.0 Iapetus (11.5mag)
00:24:44.07 +00:20:43.4 Hyperion (14.8mag)
00:26:27.00 +00:30:44.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 5 21:06 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.58555345:
14:46:46.51 -08:11:47.8 JWST
16:39:41.06 +45:52:22.5 Chandra
07:45:17.23 -29:18:28.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 5 21:06 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.58555345 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:03.68 -28:13:47.2 14.0mag P/2010 H2 (Vales)
05:00:01.14 -70:09:12.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:33.14 +31:22:31.6 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.71 +09:21:25.9 17.6mag C/2021 G2 (ATLAS)
23:07:19.01 +28:51:52.5 17.0mag C/2022 E2 (ATLAS)
04:17:52.40 +25:45:41.1 15.9mag C/2022 N2 (PANSTARRS)
09:01:51.41 +31:54:17.1 16.1mag C/2022 QE78 (ATLAS)
08:29:58.84 -01:14:41.3 17.3mag C/2022 R6 (PANSTARRS)
18:55:36.18 +17:41:08.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:32.25 -11:39:42.7 17.6mag P/2023 B1 (PANSTARRS)
09:12:54.12 -13:31:16.5 17.5mag C/2023 F3 (ATLAS)
21:43:20.78 +62:21:57.5 17.5mag C/2023 H5 (Lemmon)
19:26:28.42 -03:36:27.2 14.3mag C/2023 R1 (PANSTARRS)
21:42:39.71 +84:35:51.6 17.8mag C/2023 X2 (Lemmon)
06:14:30.57 +63:35:06.1 17.0mag C/2024 A1 (ATLAS)
04:50:48.64 +14:30:31.8 10.4mag C/2024 E1 (Wierzchos)
16:25:09.59 +04:45:37.2 17.4mag C/2024 G6 (ATLAS)
20:17:30.39 +12:39:23.1 14.7mag C/2024 J3 (ATLAS)
03:17:40.55 -23:56:24.6 16.4mag C/2024 T5 (ATLAS)
05:08:37.37 +47:51:49.9 17.7mag C/2025 J1 (Borisov)
14:19:31.45 +37:17:00.3 14.8mag C/2025 L1 (ATLAS)
03:10:12.82 -24:44:02.9 17.8mag C/2025 Q3 (ATLAS)
22:53:18.08 +19:50:13.8 10.1mag C/2025 R3 (PANSTARRS)
12:58:26.32 +02:23:06.8 17.5mag C/2025 Y1 (ATLAS)
01:29:00.09 +04:45:50.5 6.9mag C/2026 A1 (MAPS)
23:30:28.94 +35:13:14.0 14.3mag C/2026 B2 (Sun-Gao)
18:23:34.83 -10:13:23.6 12.4mag 10P/Tempel
15:13:01.72 +04:07:13.1 13.1mag 24P/Schaumasse
11:05:48.49 -01:52:03.6 15.7mag 29P/Schwassmann-Wachmann
17:56:41.91 -09:59:49.9 17.7mag 40P/Vaisala
10:38:54.73 -04:57:29.1 16.7mag 43P/Wolf-Harrington
01:33:23.34 +15:46:39.7 17.1mag 47P/Ashbrook-Jackson
06:53:09.30 +39:06:11.1 17.0mag 63P/Wild
23:16:10.00 -12:40:06.1 15.7mag 65P/Gunn
03:37:24.51 +17:41:54.3 15.8mag 76P/West-Kohoutek-Ikemura
00:43:50.89 +06:15:50.6 14.4mag 78P/Gehrels
22:32:12.42 -12:18:07.9 14.5mag 88P/Howell
01:42:52.95 +17:55:03.5 15.1mag 93P/Lovas
04:36:44.47 +31:43:19.8 16.3mag 123P/West-Hartley
08:17:50.39 +42:56:24.1 16.2mag 124P/Mrkos
02:18:03.42 +13:14:41.4 16.4mag 128P/Shoemaker-Holt
02:28:11.55 +13:14:23.8 17.5mag 131P/Mueller
00:35:21.21 +09:34:07.0 11.3mag 141P/Machholz
00:45:20.09 +01:09:38.9 11.3mag 141P-A/Machholz
23:35:57.98 -02:27:21.1 14.1mag 141P-D/Machholz
01:14:26.34 +02:49:25.4 17.9mag 141P-I/Machholz
00:34:50.54 -06:28:12.1 15.2mag 162P/SidingSpring
10:31:00.89 +31:30:44.9 17.8mag 164P/Christensen
06:18:14.31 +24:31:32.7 17.8mag 198P/ODAS
15:08:53.01 -01:12:32.3 17.3mag 210P/Christensen
21:08:34.08 -13:50:48.8 17.4mag 218P/LINEAR
17:12:32.47 -15:05:04.4 16.2mag 235P/LINEAR
05:13:26.44 +33:50:45.8 16.6mag 240P/NEAT
07:34:09.75 -06:17:59.2 17.6mag 242P/Spahr
15:45:58.05 +06:18:05.3 17.5mag 391P/Kowalski
07:30:53.38 +21:18:39.0 17.6mag 450P/LONEOS
05:21:46.30 +45:37:04.5 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 5 21:06 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 5 21:06 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 5 21:06 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
13:10:16.980 +34:24:10.02 AT 2026htp 2026-03-15.74 20.86
-rw-r--r-- 1 apache apache 30K Apr 5 21:06 tns_transients_list.txt
