This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP
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 09.3659* 20 24 31.54 +17 33 52.7 11.2 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1815041260763243392,2461139.8659,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1815041260763243392 20260409.3659 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Dauban V449,2461139.8659,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V449 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.9919+17.3288,2461139.8659,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.9919+17.3288 20260409.3659 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0375 Vul,2461139.8659,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0375 Vul 20260409.3659 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834783026412323328,2461139.8659,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834783026412323328 20260409.3659 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1822346931427650560,2461139.8659,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1822346931427650560 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1827766974003913600,2461139.8659,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827766974003913600 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BL Sge,2461139.8659,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BL Sge 20260409.3659 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821769412945285888,2461139.8659,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1821769412945285888 20260409.3659 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 40 43.97 +18 56 32.8 10.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SZ Del,2461139.8659,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SZ Del 20260409.3659 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.3279+24.5685,2461139.8659,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.3279+24.5685 20260409.3659 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 37 01.79 +17 33 04.4 13.1 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1812217611820747520,2461139.8659,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1812217611820747520 20260409.3659 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0773,2461139.8659,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0773 20260409.3659 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201009.00+233435.9,2461139.8659,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201009.00+233435.9 20260409.3659 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1856913240539076352,2461139.8659,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1856913240539076352 20260409.3659 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 13.13CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.1789+26.9453,2461139.8659,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.1789+26.9453 20260409.3659 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 27 59.17 +19 58 15.2 12.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR2 1830476479888599552,2461139.8659,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR2 1830476479888599552 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 09.3659* 20 48 43.15 +18 50 39.7 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1813226619896442752,2461139.8659,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1813226619896442752 20260409.3659 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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!
TCP 2026 04 09.3659* 20 33 16.98 +19 33 27.4 12.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 28 30.55 +18 22 09.4 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J307.1256+18.3773,2461139.8659,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.1256+18.3773 20260409.3659 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1817413525817605504,2461139.8659,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1817413525817605504 20260409.3659 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 47 41.25 +17 08 04.0 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.9284+17.1400,2461139.8659,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.9284+17.1400 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1820558227861614208,2461139.8659,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1820558227861614208 20260409.3659 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 38 47.50 +20 11 01.1 11.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1817265366625938944,2461139.8659,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1817265366625938944 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1843060489229854976,2461139.8659,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1843060489229854976 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1818032069826101632,2461139.8659,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1818032069826101632 20260409.3659 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1822263231108605056,2461139.8659,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1822263231108605056 20260409.3659 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1827203061990159616,2461139.8659,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827203061990159616 20260409.3659 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!
TCP 2026 04 09.3659* 20 49 50.88 +19 51 11.4 12.6 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1814400795235876352,2461139.8659,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1814400795235876352 20260409.3659 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 49 21.64 +19 35 34.8 12.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.3435+19.5978,2461139.8659,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.3435+19.5978 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194812.13+203010.0,2461139.8659,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194812.13+203010.0 20260409.3659 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0364 Vul,2461139.8659,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0364 Vul 20260409.3659 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J20060668+2149470,2461139.8659,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J20060668+2149470 20260409.3659 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200427.30+223749.7,2461139.8659,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200427.30+223749.7 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195742.24+182141.2,2461139.8659,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195742.24+182141.2 20260409.3659 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200635.61+233123.4,2461139.8659,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200635.61+233123.4 20260409.3659 13.16CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195835.39+214812.7,2461139.8659,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195835.39+214812.7 20260409.3659 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201523.38+214500.5,2461139.8659,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201523.38+214500.5 20260409.3659 12.04CV 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!
TCP 2026 04 09.3659* 20 43 37.45 +18 31 30.0 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J204337.75+183129.9,2461139.8659,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204337.75+183129.9 20260409.3659 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 36 00.54 +20 30 03.7 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2036008+203003,2461139.8659,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2036008+203003 20260409.3659 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204317.06+230137.0,2461139.8659,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204317.06+230137.0 20260409.3659 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6219+20.8850,2461139.8659,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6219+20.8850 20260409.3659 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SX Sge,2461139.8659,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SX Sge 20260409.3659 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195037.39+180533.2,2461139.8659,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195037.39+180533.2 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11272728,2461139.8659,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11272728 20260409.3659 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201548.28+214753.7,2461139.8659,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201548.28+214753.7 20260409.3659 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201531.19+203925.2,2461139.8659,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201531.19+203925.2 20260409.3659 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GP Sge,2461139.8659,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GP Sge 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195307.77+220145.1,2461139.8659,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195307.77+220145.1 20260409.3659 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0463 Vul,2461139.8659,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0463 Vul 20260409.3659 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1823862363372178944,2461139.8659,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1823862363372178944 20260409.3659 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201706.66+224544.6,2461139.8659,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201706.66+224544.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195754.01+193334.9,2461139.8659,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195754.01+193334.9 20260409.3659 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.3984+21.1840,2461139.8659,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.3984+21.1840 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195516.69+180743.1,2461139.8659,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195516.69+180743.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195345.54+191650.1,2461139.8659,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195345.54+191650.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WW Sge,2461139.8659,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WW Sge 20260409.3659 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204302.63+234932.3,2461139.8659,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204302.63+234932.3 20260409.3659 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201347.96+233250.8,2461139.8659,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201347.96+233250.8 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200436.11+212815.3,2461139.8659,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200436.11+212815.3 20260409.3659 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11430687,2461139.8659,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11430687 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200412.76+193424.8,2461139.8659,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200412.76+193424.8 20260409.3659 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195936.53+212145.3,2461139.8659,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195936.53+212145.3 20260409.3659 13.06CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205020.35+221736.2,2461139.8659,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205020.35+221736.2 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201426.03+170514.1,2461139.8659,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201426.03+170514.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202130.21+243252.2,2461139.8659,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202130.21+243252.2 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201750.72+193004.0,2461139.8659,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201750.72+193004.0 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2020606951135571072,2461139.8659,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2020606951135571072 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11412626,2461139.8659,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11412626 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.8275+19.3102,2461139.8659,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.8275+19.3102 20260409.3659 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!
TCP 2026 04 09.3659* 20 32 24.59 +19 29 38.6 12.1 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2032245+192934,2461139.8659,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2032245+192934 20260409.3659 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!
TCP 2026 04 09.3659* 20 30 37.66 +18 47 46.1 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203037.70+184742.3,2461139.8659,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203037.70+184742.3 20260409.3659 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200712.98+213201.3,2461139.8659,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200712.98+213201.3 20260409.3659 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2021244+205435,2461139.8659,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2021244+205435 20260409.3659 11.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202438.60+243529.5,2461139.8659,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202438.60+243529.5 20260409.3659 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200934.65+193226.5,2461139.8659,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200934.65+193226.5 20260409.3659 11.95CV 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 09.3659* 20 25 31.86 +20 03 07.8 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2025327+200310,2461139.8659,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2025327+200310 20260409.3659 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200811.65+191822.2,2461139.8659,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200811.65+191822.2 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202935.48+231558.4,2461139.8659,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202935.48+231558.4 20260409.3659 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!
TCP 2026 04 09.3659* 20 20 57.86 +20 06 52.4 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202058.02+200652.9,2461139.8659,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202058.02+200652.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2015253+241004,2461139.8659,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2015253+241004 20260409.3659 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200222.51+182348.9,2461139.8659,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200222.51+182348.9 20260409.3659 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200426.35+181944.2,2461139.8659,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200426.35+181944.2 20260409.3659 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201729.07+225753.3,2461139.8659,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201729.07+225753.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194808.52+185116.9,2461139.8659,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194808.52+185116.9 20260409.3659 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0430 Sge,2461139.8659,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0430 Sge 20260409.3659 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195946.90+183737.4,2461139.8659,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195946.90+183737.4 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2021491+233714,2461139.8659,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2021491+233714 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J201406.4+244546,2461139.8659,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J201406.4+244546 20260409.3659 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J204947+2024.7,2461139.8659,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J204947+2024.7 20260409.3659 11.04CV 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!
TCP 2026 04 09.3659* 20 36 34.35 +18 05 21.6 12.1 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203634.76+180516.5,2461139.8659,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203634.76+180516.5 20260409.3659 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.7056+18.7121,2461139.8659,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.7056+18.7121 20260409.3659 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!
TCP 2026 04 09.3659* 20 32 01.45 +18 20 33.1 11.2 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J203202+1820.5,2461139.8659,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J203202+1820.5 20260409.3659 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202650+2443.2,2461139.8659,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202650+2443.2 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J200101+2111.8,2461139.8659,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J200101+2111.8 20260409.3659 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200752.78+181336.0,2461139.8659,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200752.78+181336.0 20260409.3659 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!
TCP 2026 04 09.3659* 20 25 45.09 +19 55 45.7 12.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J20254512+1955457,2461139.8659,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J20254512+1955457 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FO Sge,2461139.8659,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FO Sge 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203717.47+250217.1,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203717.47+250217.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200447.12+213557.2,2461139.8659,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200447.12+213557.2 20260409.3659 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201456.86+243924.4,2461139.8659,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201456.86+243924.4 20260409.3659 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.4506+20.2896,2461139.8659,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.4506+20.2896 20260409.3659 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1826725289845584384,2461139.8659,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1826725289845584384 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AD Sge,2461139.8659,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AD Sge 20260409.3659 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J202215.50+234815.0,2461139.8659,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J202215.50+234815.0 20260409.3659 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200314.71+205858.3,2461139.8659,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200314.71+205858.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AZ Sge,2461139.8659,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AZ Sge 20260409.3659 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201102+1714.7,2461139.8659,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201102+1714.7 20260409.3659 11.80CV 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!
TCP 2026 04 09.3659* 20 23 40.99 +17 17 39.1 11.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2023410+171739,2461139.8659,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2023410+171739 20260409.3659 11.48CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201934.62+175914.6,2461139.8659,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201934.62+175914.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195552.93+230812.8,2461139.8659,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195552.93+230812.8 20260409.3659 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201652.93+212022.3,2461139.8659,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201652.93+212022.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200444.21+194531.8,2461139.8659,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200444.21+194531.8 20260409.3659 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201620.98+185529.6,2461139.8659,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201620.98+185529.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202558.63+244844.4,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202558.63+244844.4 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.1154+20.3063,2461139.8659,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.1154+20.3063 20260409.3659 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203345.13+260331.0,2461139.8659,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203345.13+260331.0 20260409.3659 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201806.17+201718.2,2461139.8659,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201806.17+201718.2 20260409.3659 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202620.05+215639.7,2461139.8659,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202620.05+215639.7 20260409.3659 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200344.71+242042.6,2461139.8659,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200344.71+242042.6 20260409.3659 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1810378781717085696,2461139.8659,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1810378781717085696 20260409.3659 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GV Sge,2461139.8659,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GV Sge 20260409.3659 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201516.04+221719.4,2461139.8659,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201516.04+221719.4 20260409.3659 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821990689660980864,2461139.8659,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1821990689660980864 20260409.3659 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 24 21.49 +17 58 51.3 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1815248308247559296,2461139.8659,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1815248308247559296 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200150.13+224903.6,2461139.8659,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200150.13+224903.6 20260409.3659 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11276934,2461139.8659,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11276934 20260409.3659 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 09.3659* 20 31 40.28 +17 26 06.1 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203140.53+172606.2,2461139.8659,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203140.53+172606.2 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195242.20+204120.3,2461139.8659,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195242.20+204120.3 20260409.3659 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.6673+21.9392,2461139.8659,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.6673+21.9392 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203400.78+205842.9,2461139.8659,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203400.78+205842.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195513.62+225615.6,2461139.8659,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195513.62+225615.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201352.60+201000.2,2461139.8659,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201352.60+201000.2 20260409.3659 13.13CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0427 Sge,2461139.8659,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0427 Sge 20260409.3659 10.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202916.01+253843.6,2461139.8659,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202916.01+253843.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195213.43+182006.3,2461139.8659,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195213.43+182006.3 20260409.3659 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195230.26+175116.9,2461139.8659,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195230.26+175116.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11480860,2461139.8659,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11480860 20260409.3659 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 40 44.55 +18 56 26.6 10.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SZ Del,2461139.8659,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SZ Del 20260409.3659 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201459.02+220708.4,2461139.8659,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201459.02+220708.4 20260409.3659 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11410157,2461139.8659,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11410157 20260409.3659 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201320+1811.5,2461139.8659,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201320+1811.5 20260409.3659 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 25 00.19 +19 13 05.7 11.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202500.18+191304.6,2461139.8659,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202500.18+191304.6 20260409.3659 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202415.43+225856.8,2461139.8659,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202415.43+225856.8 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J200624+1759.0,2461139.8659,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J200624+1759.0 20260409.3659 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.7534+18.3797,2461139.8659,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.7534+18.3797 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.2297+18.9654,2461139.8659,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.2297+18.9654 20260409.3659 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2005426+212026,2461139.8659,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2005426+212026 20260409.3659 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200213.55+200925.1,2461139.8659,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200213.55+200925.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2030410+242150,2461139.8659,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2030410+242150 20260409.3659 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195735.37+200456.2,2461139.8659,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195735.37+200456.2 20260409.3659 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2000567+215531,2461139.8659,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2000567+215531 20260409.3659 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194645.01+185710.3,2461139.8659,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194645.01+185710.3 20260409.3659 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195351.38+234834.2,2461139.8659,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195351.38+234834.2 20260409.3659 12.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201658.95+215231.9,2461139.8659,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201658.95+215231.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UV Vul,2461139.8659,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UV Vul 20260409.3659 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2013311+245034,2461139.8659,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2013311+245034 20260409.3659 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200815.83+235802.5,2461139.8659,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200815.83+235802.5 20260409.3659 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201540.81+213118.0,2461139.8659,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201540.81+213118.0 20260409.3659 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 25 53.94 +19 00 51.0 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821218351482336256,2461139.8659,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1821218351482336256 20260409.3659 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200820.55+233514.3,2461139.8659,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200820.55+233514.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0361 Vul,2461139.8659,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0361 Vul 20260409.3659 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195807+1728.7,2461139.8659,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J195807+1728.7 20260409.3659 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 20 54.23 +18 21 22.8 10.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UV Del,2461139.8659,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UV Del 20260409.3659 10.80CV 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!
TCP 2026 04 09.3659* 20 29 26.73 +19 53 18.7 12.2 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2029269+195319,2461139.8659,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2029269+195319 20260409.3659 12.16CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195648.02+221940.9,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195648.02+221940.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CE Sge,2461139.8659,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CE Sge 20260409.3659 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201950.08+172606.4,2461139.8659,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201950.08+172606.4 20260409.3659 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 20 42.72 +20 18 49.8 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202042.68+201852.1,2461139.8659,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202042.68+201852.1 20260409.3659 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 33 54.20 +20 27 24.2 11.6 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2033540+202724,2461139.8659,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2033540+202724 20260409.3659 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EX Sge,2461139.8659,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EX Sge 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11413222,2461139.8659,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11413222 20260409.3659 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194734.77+212501.7,2461139.8659,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194734.77+212501.7 20260409.3659 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 09.3659* 20 27 00.20 +17 20 14.8 13.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202700.34+172013.8,2461139.8659,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202700.34+172013.8 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J200853+2428.0,2461139.8659,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J200853+2428.0 20260409.3659 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DQ Vul,2461139.8659,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DQ Vul 20260409.3659 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2002469+220459,2461139.8659,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2002469+220459 20260409.3659 11.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195842.67+205422.3,2461139.8659,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195842.67+205422.3 20260409.3659 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195126+2129.6,2461139.8659,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J195126+2129.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2017225+212242,2461139.8659,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2017225+212242 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200949.38+172415.0,2461139.8659,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200949.38+172415.0 20260409.3659 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8659,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3659 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 21 44.75 +20 47 34.1 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202144.55+204732.9,2461139.8659,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202144.55+204732.9 20260409.3659 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 34 33.56 +20 18 15.2 12.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203433.65+201816.8,2461139.8659,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203433.65+201816.8 20260409.3659 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200742.74+235502.4,2461139.8659,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200742.74+235502.4 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200107.75+192534.5,2461139.8659,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200107.75+192534.5 20260409.3659 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195042.79+222944.8,2461139.8659,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195042.79+222944.8 20260409.3659 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11398205,2461139.8659,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11398205 20260409.3659 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194846.49+184446.9,2461139.8659,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194846.49+184446.9 20260409.3659 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2015382+222710,2461139.8659,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2015382+222710 20260409.3659 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201725.57+172557.2,2461139.8659,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201725.57+172557.2 20260409.3659 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MNIC V29,2461139.8659,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MNIC V29 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201224.49+181851.5,2461139.8659,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201224.49+181851.5 20260409.3659 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11268984,2461139.8659,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11268984 20260409.3659 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2001299+242760,2461139.8659,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2001299+242760 20260409.3659 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!
TCP 2026 04 09.3659* 20 23 38.98 +17 53 35.3 11.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VX Del,2461139.8659,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VX Del 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1822118125617307520,2461139.8659,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1822118125617307520 20260409.3659 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8407719,2461139.8659,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8407719 20260409.3659 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 09.3659* 20 32 28.67 +19 48 51.0 10.6 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J203229+1948.9,2461139.8659,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J203229+1948.9 20260409.3659 10.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11411631,2461139.8659,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11411631 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200214.16+174858.4,2461139.8659,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200214.16+174858.4 20260409.3659 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200848.92+243029.0,2461139.8659,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200848.92+243029.0 20260409.3659 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2029175+261731,2461139.8659,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2029175+261731 20260409.3659 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200041.55+220243.2,2461139.8659,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200041.55+220243.2 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200035.68+172808.1,2461139.8659,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200035.68+172808.1 20260409.3659 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 44 30.33 +17 39 27.6 12.1 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1269+17.6561,2461139.8659,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1269+17.6561 20260409.3659 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195630.87+232610.5,2461139.8659,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195630.87+232610.5 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GH Sge,2461139.8659,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GH Sge 20260409.3659 11.48CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201142.50+171238.8,2461139.8659,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201142.50+171238.8 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195405.32+181113.1,2461139.8659,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195405.32+181113.1 20260409.3659 12.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1814445458598178560,2461139.8659,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1814445458598178560 20260409.3659 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195627.01+193844.0,2461139.8659,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195627.01+193844.0 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BW Sge,2461139.8659,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BW Sge 20260409.3659 12.49CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J200331+1913.3,2461139.8659,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J200331+1913.3 20260409.3659 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8538508,2461139.8659,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8538508 20260409.3659 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2001131+192937,2461139.8659,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2001131+192937 20260409.3659 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203019.50+210650.2,2461139.8659,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203019.50+210650.2 20260409.3659 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2003017+195720,2461139.8659,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2003017+195720 20260409.3659 12.16CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11395442,2461139.8659,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11395442 20260409.3659 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2003518+180454,2461139.8659,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2003518+180454 20260409.3659 11.45CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200634.22+202142.4,2461139.8659,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200634.22+202142.4 20260409.3659 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7731+19.5606,2461139.8659,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7731+19.5606 20260409.3659 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11402603,2461139.8659,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11402603 20260409.3659 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!
TCP 2026 04 09.3659* 20 37 33.17 +20 03 17.4 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2037332+200317,2461139.8659,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2037332+200317 20260409.3659 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200807.70+173719.1,2461139.8659,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200807.70+173719.1 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202143.47+265337.4,2461139.8659,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202143.47+265337.4 20260409.3659 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EL Vul,2461139.8659,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EL Vul 20260409.3659 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 32 04.56 +18 24 25.3 11.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AC Del,2461139.8659,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Del 20260409.3659 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2040288+221253,2461139.8659,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2040288+221253 20260409.3659 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195642.91+200956.0,2461139.8659,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195642.91+200956.0 20260409.3659 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202441+2239.0,2461139.8659,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202441+2239.0 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195521.58+202622.6,2461139.8659,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195521.58+202622.6 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CO Sge,2461139.8659,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CO Sge 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200158.31+212501.9,2461139.8659,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200158.31+212501.9 20260409.3659 13.06CV 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!
TCP 2026 04 09.3659* 20 33 48.60 +20 48 07.2 9.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J203348+2048.1,2461139.8659,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J203348+2048.1 20260409.3659 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194713.91+210539.2,2461139.8659,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194713.91+210539.2 20260409.3659 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2049309+233459,2461139.8659,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2049309+233459 20260409.3659 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11401034,2461139.8659,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11401034 20260409.3659 11.48CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202123.54+220146.9,2461139.8659,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202123.54+220146.9 20260409.3659 12.41CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200539.01+213229.6,2461139.8659,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200539.01+213229.6 20260409.3659 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 32 06.82 +20 39 07.1 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2032074+203906,2461139.8659,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2032074+203906 20260409.3659 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 25 29.98 +20 44 57.3 11.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2025299+204456,2461139.8659,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2025299+204456 20260409.3659 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FM Sge,2461139.8659,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FM Sge 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195256.49+233132.9,2461139.8659,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195256.49+233132.9 20260409.3659 12.13CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194718.16+201808.3,2461139.8659,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194718.16+201808.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0226,2461139.8659,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0226 20260409.3659 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11278755,2461139.8659,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11278755 20260409.3659 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3659* 20 27 19.96 +18 49 58.7 11.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2027203+184959,2461139.8659,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2027203+184959 20260409.3659 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11276525,2461139.8659,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11276525 20260409.3659 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!
TCP 2026 04 09.3659* 20 24 30.66 +20 19 50.2 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202430.48+201949.0,2461139.8659,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202430.48+201949.0 20260409.3659 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201322.98+210320.7,2461139.8659,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201322.98+210320.7 20260409.3659 11.48CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200126.98+211552.9,2461139.8659,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200126.98+211552.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8414789,2461139.8659,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8414789 20260409.3659 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1827256830651730560,2461139.8659,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827256830651730560 20260409.3659 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201540.83+234746.9,2461139.8659,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201540.83+234746.9 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DU Sge,2461139.8659,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DU Sge 20260409.3659 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0227,2461139.8659,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0227 20260409.3659 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AI Sge,2461139.8659,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AI Sge 20260409.3659 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200324.90+231951.0,2461139.8659,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200324.90+231951.0 20260409.3659 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11271657,2461139.8659,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11271657 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1843575374208730752,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1843575374208730752 20260409.3659 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 09.3659* 20 47 59.39 +18 18 46.3 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J204759+1818.6,2461139.8659,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J204759+1818.6 20260409.3659 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821474846933788032,2461139.8659,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1821474846933788032 20260409.3659 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11407212,2461139.8659,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11407212 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194630+1911.3,2461139.8659,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194630+1911.3 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11406915,2461139.8659,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11406915 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0342,2461139.8659,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0342 20260409.3659 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!
TCP 2026 04 09.3659* 20 26 04.45 +20 46 13.2 12.2 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2026060+204616,2461139.8659,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2026060+204616 20260409.3659 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203112.67+261227.1,2461139.8659,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203112.67+261227.1 20260409.3659 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8659,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3659 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202402.83+245853.5,2461139.8659,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202402.83+245853.5 20260409.3659 13.16CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200900.19+201828.4,2461139.8659,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200900.19+201828.4 20260409.3659 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195504.35+225554.8,2461139.8659,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195504.35+225554.8 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1947246+235035,2461139.8659,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1947246+235035 20260409.3659 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N021121012-1-86-2,2461139.8659,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N021121012-1-86-2 20260409.3659 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202215.93+212401.3,2461139.8659,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202215.93+212401.3 20260409.3659 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1823042578698664704,2461139.8659,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1823042578698664704 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202257.62+223801.8,2461139.8659,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202257.62+223801.8 20260409.3659 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194957.14+190234.7,2461139.8659,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194957.14+190234.7 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200847.13+182645.5,2461139.8659,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200847.13+182645.5 20260409.3659 11.67CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195338.90+240560.0,2461139.8659,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195338.90+240560.0 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2036217+245842,2461139.8659,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2036217+245842 20260409.3659 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2013054+201435,2461139.8659,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2013054+201435 20260409.3659 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8659,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.9699+25.3148,2461139.8659,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.9699+25.3148 20260409.3659 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201720.83+235019.9,2461139.8659,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201720.83+235019.9 20260409.3659 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.9400+23.8167,2461139.8659,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.9400+23.8167 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1828746467054703744,2461139.8659,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1828746467054703744 20260409.3659 12.49CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.8101+19.7472,2461139.8659,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.8101+19.7472 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200135.35+184446.0,2461139.8659,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200135.35+184446.0 20260409.3659 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DE Vul,2461139.8659,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Vul 20260409.3659 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200631.99+192739.3,2461139.8659,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200631.99+192739.3 20260409.3659 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461139.86634435 09.04.2026 08:47:22.152 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 91
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 24501
Objects passed selection criteria: 24458
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 21016.8
Average stars matched: 20340.8 (96.7835 %)
Memory usage VmPeak: 127252 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 03:53:21 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461139.86634435 09.04.2026 08:47:22.152 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 573
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 72 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): 214029
Objects passed selection criteria: 213441
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 163444
Average stars matched: 156794 (95.9316 %)
Memory usage VmPeak: 2032300 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 04:00:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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: 2461139.86544341
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits'
wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:31.387 +22:00:51.32
Angular distance between the image centers 0.0139 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:28.459 +22:00:09.93
Angular distance between the image centers 0.0022 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 20:18:31.387 +22:00:51.32
Second-epoch second image center 20:18:28.459 +22:00:09.93
Angular distance between the image centers 0.01613 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/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.fJiR7wz8Jb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.OIIdxiAGTK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.uaYr4NRTMl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits &> /tmp/tmp.6u9jhaN39W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 24638 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6627 to 313.2570 deg, Dec +16.3767 to +27.3369 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 295.6627 to 313.2570 deg, Dec 16.3767 to 27.3369 deg
Loaded 24193 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): 13464 out of 14549 total matches.
Matched with Tycho-2 14549 out of 24638 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758582
a=0.000000 b=1.000000 c=22.758582
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 90 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
4.8 pix fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
4.8 pix fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Limiting magnitude estimates:
14.8 mag. Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.8 mag. Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
14.0 mag. fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
14.0 mag. fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.5 (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.fJiR7wz8Jb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2463, passed=24638
Got 24638 stars (including 22152 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 24638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.OIIdxiAGTK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2477, passed=24779
Got 24779 stars (including 22281 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 24779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.uaYr4NRTMl (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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1013, passed=17529
Got 17529 stars (including 16511 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 17529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 17139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 17139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 17118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.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.6u9jhaN39W (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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1018, passed=17650
Got 17650 stars (including 16628 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat
util/solve_plate_with_UCAC5 got 17650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 17256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 17256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 17256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 934 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits -region wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits'
Preparing the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32325.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 7s
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Considering the candidate 31520_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 31520_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 31622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:33.29 +19:06:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31797_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31797_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:26:15.16 +20:27:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31899_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31899_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:12.53 +18:12:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31901_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31901_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:44.28 +21:26:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31909_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31909_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:18.78 +18:25:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31928_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31928_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:50:10.03 +21:13:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31953_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31953_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:07.32 +20:47:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31988_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31988_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:54.64 +23:29:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:22:34.98 +17:37:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31999_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31999_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:20.72 +20:56:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32032_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32032_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32054_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32054_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:45:37.88 +22:51:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32102_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32102_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:08.85 +26:48:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32110_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32110_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32111_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32111_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:41:52.23 +19:54:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32117_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32117_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32119_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32119_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:01:00.97 +21:11:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 1.293 1823810209620152320 300.25435005438 +21.19784022599 10.5533 9.2771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32123_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32123_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:46:30.72 +19:11:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 5.403 1824647895716338176 296.62655117249 +19.18893883607 10.6165 9.1979 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32124_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32124_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 32166_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32166_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:26:50.26 +24:43:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 3.772 1831653781954279808 306.70921591518 +24.72114301849 10.8737 9.5286 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32169_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32169_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:30.80 +17:51:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32171_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32171_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:00:46.09 +20:34:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32172_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32172_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:01.13 +18:45:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32183_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32183_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:28.60 +20:44:19.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)
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Considering the candidate 32184_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32184_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32193_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32193_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:02:56.83 +21:33:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.741 1823916862245809152 300.73668064239 +21.55198361659 11.4982 9.8484 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32196_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32196_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:24.83 +21:34:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.710 1826697458450648320 298.60396731414 +21.57981772082 11.2266 10.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32205_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32205_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:08:52.54 +21:23:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:50.22 +22:10:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 5.402 1827575899514936448 297.20763313854 +22.17053854947 10.6418 9.5563 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32214_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32214_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:54.73 +19:46:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.584 1824781422004963200 297.47733289596 +19.77537347922 10.4423 8.8953 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32226_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32226_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:45.39 +19:02:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.526 1822946680675137664 299.68898707917 +19.04676744594 10.8288 9.5159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32227_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32227_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:11.98 +17:31:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32235_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32235_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:39.91 +23:34:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 4.016 1833230515998168576 301.41683446658 +23.57994300907 11.2807 10.1822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32240_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32240_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:14.33 +21:26:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 0.485 1826691686013991680 298.30969419365 +21.44118961098 10.9397 9.6892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32246_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32246_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:48.37 +25:33:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32253_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32253_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:19.17 +17:24:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32259_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32259_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:04:05.12 +21:14:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 3.228 1823847352491490560 301.02217739026 +21.23493009874 11.2846 10.1637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:23.16 +21:34:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 4.899 1827482475387121152 297.34606796540 +21.57314441396 11.7478 10.8761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32283_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32283_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:32.59 +17:17:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:31.76 +23:09:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.576 1830464007302657280 302.88298670575 +23.15461089120 11.3524 10.3896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32311_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32311_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:45:55.40 +23:20:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.436 2020055339892337152 296.48013329605 +23.34898931601 10.7992 9.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32318_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32318_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:56.66 +19:04:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 4.380 1824588938752717696 296.98591342695 +19.07073367808 11.6704 10.9895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32325_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32325_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32330_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32330_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:53.99 +19:17:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.992 1821696948289514752 297.97481112099 +19.28692855809 11.0455 9.6960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32337_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32337_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:14.75 +19:43:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32341_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32341_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:37.50 +20:08:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.095 1826491403097731200 297.40574197751 +20.13938873199 10.9027 9.5555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:55.39 +25:02:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.280 1833790579732068992 303.23205700861 +25.04361309319 12.0408 11.5936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32343_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32343_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:46.74 +18:44:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 4.318 1824565952085399040 297.19373908094 +18.74633292497 10.7719 9.4583 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32344_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32344_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:00.09 +26:25:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.627 2027079118941665152 298.50086992087 +26.41819873211 11.8298 11.3584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32346_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32346_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 32353_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32353_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:57:53.00 +23:50:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 3.411 1834123559955105920 299.47170851875 +23.84890947804 10.9773 9.6856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32358_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32358_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:45:40.68 +24:11:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.958 2020531321038275584 296.41947643750 +24.19993185130 11.4998 10.5430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32361_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32361_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:49.41 +22:33:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.667 1827940662497870976 298.45593086546 +22.56601140458 10.8729 9.5156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32366_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32366_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:24.92 +22:56:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.475 1833128055255009280 301.35427836173 +22.94661421522 11.0858 9.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:31.89 +26:31:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.979 2027236933220132480 299.63317852463 +26.51848424174 11.8607 11.3735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:28.75 +20:28:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 1.223 1825064340091834112 296.86943153705 +20.46998834833 11.3941 10.3247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32402_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32402_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:31.97 +26:01:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.138 2026855853671795456 298.38321159672 +26.02564936002 11.1938 9.9386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:55:55.68 +23:41:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.855 1828160560484882688 298.98224140210 +23.68758686584 11.9930 11.3353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32416_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32416_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:46:54.98 +22:30:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 3.204 1827787796006264064 296.72812151676 +22.51127375004 11.6474 10.6537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32417_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32417_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:59:36.48 +25:55:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 1.212 1835014233101467008 299.90187819254 +25.91801266522 11.5603 10.4365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32422_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32422_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:00:34.43 +20:53:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.950 1823786840667242880 300.14378705459 +20.88908500642 11.6366 10.9310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32423_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32423_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:24.13 +21:52:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.098 1827130391140862976 298.35083020452 +21.88150725926 11.3255 10.2251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:40.13 +20:17:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.875 1826497824030118400 297.41721348294 +20.29559025343 12.0077 11.5714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32429_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32429_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:55:39.01 +23:28:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 1.349 1828148264033304704 298.91294878790 +23.48102259621 11.6009 10.6915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32431_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32431_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:55:46.21 +21:07:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07026_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 07026_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:45.97 +19:29:32.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03077_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 03077_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 12160_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 12160_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:35.61 +21:35:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14238_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 14238_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:47:12.10 +22:39:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11261_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 11261_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:35:30.03 +21:23:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22014_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 22014_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:28:01.84 +26:03:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03522_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 03522_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:14:23.64 +18:06:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30326_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 30326_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:08:04.69 +20:50:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 06021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:43:58.15 +19:14:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12505_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 12505_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:02:57.21 +21:41:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05033_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 05033_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:38:09.29 +18:50:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00645_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 00645_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:43:04.63 +17:05:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06233_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 06233_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:13.05 +19:15:22.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14892_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 14892_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:17.48 +22:48:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31032_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31032_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:24.32 +17:59:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.868 1821874691180192896 301.60127477820 +17.98323418375 10.6399 9.2399 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02718_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 02718_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05273_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 05273_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10605_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 10605_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:34:28.99 +21:05:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07233_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 07233_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:00.19 +19:34:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11189_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 11189_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:40.42 +21:24:33.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10672_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 10672_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:38:31.21 +21:12:02.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02996_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 02996_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:45:28.07 +18:05:25.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 03374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:37:54.59 +18:16:10.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 25s
Prepared the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:05:15.92 +17:40:53.4
20:04:21.94 +17:48:39.9
20:40:43.97 +18:56:32.8
20:24:31.54 +17:33:52.7
19:47:50.55 +17:51:15.5
19:51:56.44 +17:20:02.8
20:27:28.19 +24:17:20.6
20:02:28.78 +25:37:35.8
20:08:07.41 +18:46:14.8
19:47:34.74 +22:14:35.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:31.387 +22:00:51.32
Angular distance between the image centers 0.0139 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:28.459 +22:00:09.93
Angular distance between the image centers 0.0022 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 20:18:31.387 +22:00:51.32
Second-epoch second image center 20:18:28.459 +22:00:09.93
Angular distance between the image centers 0.01613 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/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.mmURIHTIAK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.m65xhzyBW4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.OJTuASvwRp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits &> /tmp/tmp.NwqLlcxldu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 232861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6471 to 313.2612 deg, Dec +16.3395 to +27.3423 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 295.6471 to 313.2612 deg, Dec 16.3395 to 27.3423 deg
Loaded 24297 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): 12337 out of 17496 total matches.
Matched with Tycho-2 17496 out of 232861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.561146
a=0.000000 b=1.000000 c=22.561146
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 527 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
1.9 pix Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
4.2 pix fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
4.2 pix fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Limiting magnitude estimates:
14.9 mag. Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.9 mag. Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
14.0 mag. fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
14.0 mag. fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.2 (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.mmURIHTIAK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=33174, passed=232816
Got 232816 stars (including 199295 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 232816 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228423 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.m65xhzyBW4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32901, passed=232172
Got 232172 stars (including 198927 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 232172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.OJTuASvwRp (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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=13116, passed=96665
Got 96665 stars (including 83482 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 96665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 94894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 94897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 94897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 941 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.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.NwqLlcxldu (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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=13160, passed=97264
Got 97264 stars (including 84027 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat
util/solve_plate_with_UCAC5 got 97264 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 95567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 95565 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 95564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 941 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits -region wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_Vul-02-Q1b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_Vul-02-Q1b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-46-04_20.00sec_-4.90C_LIGHTs_0226.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.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_2026-04-09_CI_Vul-02-Q1b1x1_034812_TTUQ1b1x1_8477_RJAu5itP/wcs_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227.fits
Preparing the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out147316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out19631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out261796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out266943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out46462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out244533.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out264288.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out264448.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out08392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out180965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out206756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out230406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99342.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 145s
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: 152s
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Considering the candidate 264265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:38.91 +23:17:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.705 1833140871437325568 301.66099031428 +23.29725076969 14.2870 13.4624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264266_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264266_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:28:33.21 +23:12:14.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 264282_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264282_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 264283_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264283_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:57:54.14 +21:02:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 5.870 1826793012871850368 299.47526020492 +21.03864765779 13.6012 12.9834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264286_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264286_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:45:53.01 +26:03:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.946 1844050053991934336 311.47176944718 +26.05901182279 13.3847 12.8502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264288_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264288_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:41.17 +23:52:41.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264300_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264300_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264301_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264301_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:42.30 +23:55:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.043 1833574525694267392 302.92571113263 +23.92509271678 13.7718 12.8892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264302_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264302_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:59.43 +23:24:41.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264305_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264305_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264308_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264308_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:40:59.78 +19:05:14.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264314_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264314_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264315_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264315_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:48.49 +20:34:33.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 264317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:51:50.47 +25:43:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.801 1843830697124830592 312.95892007135 +25.72174833148 12.6971 12.1790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264319_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264319_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264321_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264321_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:57:17.54 +17:59:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.340 1820570704764274944 299.32407034544 +17.98891043459 12.9017 12.4545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264324_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264324_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:02.59 +19:47:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.884 1824954938675967616 297.01222554294 +19.79941301183 13.4269 12.8899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264334_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264334_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 264341_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264341_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:46:00.77 +19:34:24.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 264342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264348_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264348_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:11.84 +19:35:23.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 264350_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264350_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:39.03 +26:32:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.175 1835121607279194880 301.41405358046 +26.54084195339 13.2983 12.1058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264352_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264352_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:45:13.22 +22:35:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 264355_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264355_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:45:20.63 +25:14:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 5.019 1843566234518453376 311.33745590256 +25.24789242677 13.1431 12.6633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264360_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264360_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264365_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264365_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264368_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264368_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264369_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264369_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:08:37.39 +19:21:04.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 264372_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264372_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:14:56.59 +22:53:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.600 1830262929795140480 303.73622137800 +22.89695161571 13.0493 12.2147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264373_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264373_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:04.10 +22:08:41.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 264375_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264375_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:24:45.58 +21:37:33.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 264378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:51:03.87 +24:40:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.796 1842903018548515328 312.76789445525 +24.68024731656 12.3726 11.3352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264381_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264381_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:27:51.98 +19:39:35.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 264382_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264382_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:25.38 +19:00:41.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 264383_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264383_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:49.30 +21:58:30.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 264384_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264384_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:18.27 +20:49:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 264386_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264386_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:18:32.69 +22:04:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 264387_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264387_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:01:58.89 +21:14:35.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 264388_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264388_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:38.85 +19:14:47.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
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Considering the candidate 264390_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264390_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:35:04.66 +17:58:49.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 264394_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264394_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 264402_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264402_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264407_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264407_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:16:08.54 +24:33:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.545 1832199071008292992 304.03515761387 +24.55890840179 13.0445 12.2301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264408_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264408_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264417_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264417_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:46:16.42 +16:59:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.927 1811209664596423040 311.56803973152 +16.98549349276 11.8341 11.3254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264422_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264422_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:32:45.21 +19:21:53.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 264429_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264429_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:33:31.03 +16:56:08.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)
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Considering the candidate 264436_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264436_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:04.07 +21:47:31.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 264437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264440_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264440_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264443_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264443_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264444_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264444_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264445_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264445_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:46:58.93 +19:16:48.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)
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Considering the candidate 264448_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264448_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:58.19 +21:10:33.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 264449_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264449_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264452_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264452_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:00:45.20 +17:13:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.263 1820283453030883968 300.18828650674 +17.22962203363 12.5095 11.2331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264454_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264454_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:46:49.57 +26:15:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 264457_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264457_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:48:07.21 +20:04:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.212 1814468720141054336 312.03044555086 +20.06610902591 12.3086 11.5852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264458_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264458_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264462_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264462_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264464_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264464_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 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 264466_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264466_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:34:16.77 +22:11:13.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 264471_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264471_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:08.90 +20:01:20.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)
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Considering the candidate 264478_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264478_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:47:05.73 +25:03:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 5.574 1843736005982351488 311.77517743847 +25.06722493703 12.3544 10.5798 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264479_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264479_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:04.96 +18:30:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 4.858 1810291606751870592 303.02167427258 +18.51343602886 12.4785 12.0350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264481_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264481_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:36.73 +18:12:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264484_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264484_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264491_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264491_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:49:20.03 +17:30:56.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)
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Considering the candidate 264492_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264492_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:23:54.57 +21:48:28.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 264494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:40:24.47 +19:01:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)
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Considering the candidate 264495_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264495_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:57:34.72 +21:45:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.747 1826902964038935808 299.39535092574 +21.76436681897 12.4632 11.5154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264496_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264496_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 264498_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 264498_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 264503_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 264503_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:36:15.87 +16:48:54.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 265181_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 265181_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:30.06 +18:29:56.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 265209_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 265209_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:10:43.48 +27:12:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265336_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 265336_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:38.72 +17:51:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265687_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 265687_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 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 265756_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 265756_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 265875_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 265875_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 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 266000_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266000_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:13.33 +17:43:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266195_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 266195_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 266206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:55:06.15 +26:46:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.522 2027469518601525120 298.77577686999 +26.78021788273 12.6985 12.1941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266232_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266232_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:39.54 +22:27:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.770 1827925956529136128 298.16583202005 +22.45608892717 12.6682 12.1413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266234_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266234_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:57:32.37 +17:44:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266270_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266270_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:03:52.12 +21:04:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266278_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266278_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:27:00.35 +22:20:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266322_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266322_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:40:42.32 +26:03:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:11.53 +20:23:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266415_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266415_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:56.73 +26:49:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.106 2027146502704732800 297.73577586669 +26.82751488006 13.3300 12.8040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266428_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266428_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:02.95 +19:27:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.499 1822641321355637120 301.26301314749 +19.46097093970 12.2320 10.7835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 266437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 266456_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266456_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:14:42.32 +26:25:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266553_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266553_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:03:07.86 +25:17:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266672_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266672_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:22.63 +26:28:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.337 2027083242110265088 298.34500187056 +26.48175744937 12.8986 12.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266753_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266753_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:04.52 +18:54:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266802_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266802_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 266825_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266825_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:04:17.39 +22:05:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.426 1829964519792166656 301.07264066586 +22.08329199226 13.0207 11.0669 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266916_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266916_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 266922_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266922_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:46:38.79 +19:10:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266927_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266927_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:22:44.24 +24:03:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266935_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 266935_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 266943_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 266943_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:59:15.77 +21:53:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.104 1826989889843029888 299.81672450232 +21.88497547083 11.8893 10.3460 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267001_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267001_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 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 267203_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267203_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:33.40 +18:40:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267207_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 267207_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 267267_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267267_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:28.95 +21:11:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.049 1826669828875155200 298.61996658171 +21.19622246434 12.1233 10.5083 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267305_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267305_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:59:39.41 +19:29:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 5.633 1823057830104749312 299.91344183879 +19.48541776682 12.4136 10.9942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:03:59.35 +21:37:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.012 1823930022026222208 300.99622302350 +21.61906043123 12.0498 9.9921 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267586_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267586_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:20.08 +25:27:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267864_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267864_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:15.64 +23:20:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.472 1828227939933496320 298.06440135074 +23.34463300713 12.3224 10.7748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267899_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 267899_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:55.39 +24:47:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.381 2020677178129357696 297.47995834881 +24.78942800042 12.1366 10.4175 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267931_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 267931_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 267998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 267998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 268020_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268020_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:21.11 +25:37:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.951 1835337279039488640 303.83865596565 +25.63370484528 12.2502 10.7741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268045_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268045_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:14:25.10 +20:14:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.550 1828572568108492416 303.60530222617 +20.24668902240 13.5753 11.6627 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268068_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268068_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:33.17 +20:57:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268147_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268147_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:23.63 +23:22:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.889 1833165777934458752 301.84918324360 +23.37049003309 11.8257 10.0511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268157_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268157_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:17:09.44 +25:53:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268163_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268163_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:48.68 +21:19:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.530 1829665864943626112 301.95324561766 +21.32434835618 13.6985 11.5196 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268165_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268165_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:05.56 +21:59:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.329 1827138740557721216 298.52362146115 +21.99282285515 13.3986 10.8343 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268190_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268190_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:36:42.10 +22:54:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.112 1819015681761720192 309.17604858859 +22.90326827711 13.3685 11.5354 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268206_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:52.30 +18:40:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.344 1821559917308034688 297.46726413780 +18.67476769529 12.7937 11.2737 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268249_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268249_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:37.38 +22:59:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268262_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268262_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:08.86 +24:59:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.159 1833930698741408512 301.78745652604 +24.98720790819 14.0314 11.8947 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268311_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268311_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:21.76 +23:06:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.920 1828078926077251712 299.09121153924 +23.10273799201 12.8931 11.4132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268330_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268330_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:04:48.64 +24:09:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.095 1833454919445628544 301.20301271709 +24.15407202697 13.3637 11.8489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268349_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268349_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:28:51.46 +24:38:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.108 1831640072418337280 307.21479137084 +24.64297787502 12.7241 11.0977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268377_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268377_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:02:27.50 +22:57:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.643 1833070296548092672 300.61507809394 +22.96280327597 12.1493 10.4951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268383_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268383_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:10:50.23 +25:40:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268405_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 268405_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 268406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:13:57.30 +23:39:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.580 1830596184904901120 303.48943739637 +23.66373099509 12.4077 10.9220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:13:38.46 +26:37:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.907 1835724105293050496 303.41081453976 +26.62143303101 12.5123 10.9650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 268425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 268437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268437_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:48.14 +18:22:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268450_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268450_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:37:11.28 +25:44:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268479_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268479_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:22:09.71 +22:22:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.752 1829481971611691392 305.54111665065 +22.38315701473 12.7338 11.2440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268488_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268488_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:04:56.65 +25:04:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 2.600 1834690697482104704 301.23667092913 +25.06730482120 12.2697 10.6103 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:05.64 +26:11:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.749 1835611714584760064 303.02435005619 +26.18412546047 12.7592 11.2617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268510_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268510_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:10:00.92 +25:37:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.150 1834071230066712704 302.50449344446 +25.63320058619 12.9645 10.8989 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268526_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268526_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:34.07 +18:27:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.653 1821963408028616320 301.89194254414 +18.46645862224 12.8812 11.3210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268547_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268547_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:55.00 +21:55:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.174 1827096512444960640 299.22970593648 +21.93172696878 12.7715 11.2384 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:03:28.06 +23:29:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.395 1833392586567186432 300.86757935472 +23.49560394913 12.8208 11.3103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268592_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 268592_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:10:44.15 +26:09:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.664 1835601986464522368 302.68433578320 +26.16161984486 12.5375 11.0217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35712_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 35712_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:37:54.58 +18:16:11.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 186157_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 186157_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:44:52.40 +25:16:06.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 26392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 26392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:00:03.65 +17:31:02.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:45:28.07 +18:05:25.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115791_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 115791_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:38:31.20 +21:12:02.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 146040_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 146040_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 26166_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 26166_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:21.53 +17:47:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 229413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 229413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:16.09 +25:35:24.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40832_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 40832_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 81811_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 81811_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:09.94 +19:59:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165805_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 165805_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 127966_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 127966_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 171440_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 171440_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:53.77 +23:36:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182867_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 182867_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:16:47.27 +24:40:09.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 168079_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 168079_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:30.42 +23:30:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 116317_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:40.41 +21:24:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 109611_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 109611_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:03.76 +21:08:05.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121154_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 121154_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:16:19.91 +21:35:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 122219_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 122219_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 37308_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 37308_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 86733_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 86733_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 151000_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 151000_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 104483_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 104483_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 42062_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 42062_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 36968_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 36968_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 159499_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 159499_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 123073_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 123073_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 93177_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 93177_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 105563_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 105563_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 135793_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 135793_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 125528_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 125528_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 112673_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 112673_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 87318_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 87318_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:26:15.16 +20:27:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26281_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 26281_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:04:21.95 +17:48:39.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 146126_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 146126_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 69805_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 69805_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 112352_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 112352_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 101467_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 101467_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:08:04.72 +20:50:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36089_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 36089_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 55158_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 55158_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:34.46 +18:52:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.478 1821650700077959680 297.89315133085 +18.87726749050 11.2994 9.7535 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 64235_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 64235_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 52279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 52279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 168793_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 168793_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 164795_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 164795_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 80328_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 80328_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 117607_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 117607_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 138172_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 138172_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 68140_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 68140_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 116297_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 116297_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 81473_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 81473_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:07.31 +20:10:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.673 1822741759182006400 302.78091154852 +20.16915893803 12.3611 10.9036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58059_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 58059_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:13.06 +19:15:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134299_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 134299_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 51876_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 51876_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:42.81 +19:04:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.482 1816189528863801856 305.17899524688 +19.07280752138 12.6235 11.0764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 08392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 199263_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 199263_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 62921_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 62921_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 193881_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 193881_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 104385_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 104385_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 249208_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 249208_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:06.10 +22:13:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.862 1829829000666517632 302.77591851884 +22.23092199198 11.7532 10.2134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65884_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 65884_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 98125_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 98125_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:07.32 +20:47:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61062_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 61062_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 44248_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 44248_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 101229_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 101229_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:20.74 +20:55:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118312_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 118312_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 99221_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 99221_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 198738_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 198738_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 66187_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 66187_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 76225_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 76225_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 60278_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 60278_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 156561_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 156561_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 261796_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 261796_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:23:32.84 +24:07:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.278 1831983498004605440 305.88750825169 +24.13286749884 12.5970 11.2419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78234_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 78234_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 177164_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 177164_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 40357_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 40357_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 38181_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 38181_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 150770_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 150770_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 56167_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 56167_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 05957_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 05957_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:47:55.90 +17:04:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59815_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 59815_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 46681_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 46681_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 165363_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 165363_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 194531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 194531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 85320_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 85320_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 151265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 151265_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:59.30 +22:56:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.181 1830439989845667328 302.99740590396 +22.94074885446 11.6976 10.1061 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 27567_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 27567_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 47767_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 47767_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 34052_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 34052_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 196850_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 196850_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 112158_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 112158_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 34577_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 34577_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 72574_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 72574_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 38489_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 38489_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 191409_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 191409_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 120980_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 120980_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 196634_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 196634_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 90646_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 90646_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 121667_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 121667_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 177425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 177425_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:05:57.45 +24:05:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.288 1833439659411491200 301.48979699615 +24.09369997177 12.2249 10.7361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25046_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 25046_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 168846_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 168846_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 105089_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 105089_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 24622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 24622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 12349_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 12349_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 11773_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 11773_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 26782_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 26782_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 53589_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 53589_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:03.61 +19:07:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160650_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 160650_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 111056_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 111056_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 73047_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 73047_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 49430_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 49430_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 194740_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 194740_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 87078_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 87078_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 222133_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 222133_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 83413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 83413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 125331_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 125331_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 182797_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 182797_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 57832_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 57832_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:24:58.31 +19:20:08.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)
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Considering the candidate 43618_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 43618_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 108971_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 108971_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 135285_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 135285_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 221934_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 221934_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:28:01.83 +26:03:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25597_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 25597_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 45427_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 45427_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:38:09.29 +18:50:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26115_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 26115_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 151204_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 151204_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 157380_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 157380_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 226911_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 226911_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:20:15.74 +25:45:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13578_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 13578_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 101804_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 101804_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 128553_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 128553_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 99342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 99342_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 156386_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 156386_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 80873_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 80873_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 64164_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 64164_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 176737_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 176737_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:52.12 +23:55:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.623 1834169735132361728 299.21788192105 +23.92906805749 12.4387 10.9343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 230406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 230406_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 41809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 41809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 30727_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 30727_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 159224_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 159224_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 166677_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 166677_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:42:21.98 +23:43:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47399_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 47399_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 168011_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 168011_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:55:26.38 +23:27:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.103 1828148160954125184 298.86042354507 +23.45467940902 12.0521 10.4884 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131058_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 131058_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 31689_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 31689_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 08587_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 08587_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32996_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32996_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 55371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 55371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 37789_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 37789_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:19:18.77 +18:25:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150368_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 150368_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 29936_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 29936_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 36205_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 36205_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 51809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 51809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 114151_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 114151_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 83792_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 83792_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 179954_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 179954_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 83475_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 83475_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 55658_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 55658_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:43:58.14 +19:14:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112844_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 112844_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:13.01 +20:58:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130484_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 130484_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 59161_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 59161_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 175494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 175494_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 125118_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 125118_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 171187_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 171187_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 192691_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 192691_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 151163_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 151163_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:17.47 +22:48:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174782_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 174782_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 115874_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 115874_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 49745_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 49745_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 125576_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 125576_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:02:57.46 +21:41:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71093_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 71093_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 21002_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 21002_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 166845_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 166845_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 152531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 152531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 20783_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 20783_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 35916_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 35916_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 71589_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 71589_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 141360_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 141360_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 148186_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 148186_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:01.16 +22:29:33.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)
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Considering the candidate 208362_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 208362_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:25:08.85 +26:48:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30799_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 30799_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 18501_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 18501_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:22:34.98 +17:37:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15071_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 15071_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 106828_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 106828_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:50:10.02 +21:13:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83518_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 83518_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 158562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 158562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:45:37.91 +22:51:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86212_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 86212_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 27316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 27316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 98674_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 98674_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 123105_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 123105_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 11655_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 11655_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 198809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 198809_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 67850_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 67850_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 151021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 151021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 134014_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 134014_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 120622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 120622_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:06:35.79 +21:35:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142930_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 142930_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:47:12.09 +22:39:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104928_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 104928_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 123868_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 123868_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 112012_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 112012_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 15786_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 15786_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 111392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 111392_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:35:30.02 +21:23:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121456_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 121456_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 31296_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 31296_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:14:23.64 +18:06:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178948_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 178948_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:37:57.27 +24:20:30.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 227312_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 227312_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 95647_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 95647_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 81493_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 81493_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 173628_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 173628_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 248021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 248021_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:17:17.67 +20:00:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.423 1828506017605070720 304.32433848184 +20.00652505432 12.4124 10.8446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65306_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 65306_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 147712_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 147712_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 82624_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 82624_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32252_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32252_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:30.68 +17:51:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53621_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 53621_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 139024_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 139024_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 14936_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 14936_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 97640_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 97640_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 35689_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 35689_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 75668_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 75668_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 197143_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 197143_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 24518_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 24518_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 45126_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 45126_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 170272_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 170272_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 178649_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 178649_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:27:28.17 +24:17:19.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 114135_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 114135_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:15:20.21 +21:27:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.880 1828943004758195712 303.83538911183 +21.45707134216 12.7070 11.3075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69370_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 69370_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:12:00.19 +19:34:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95991_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 95991_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:44:14.63 +20:49:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69653_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 69653_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 10144_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 10144_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 26772_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 26772_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 198120_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 198120_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 112934_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 112934_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:44.27 +21:26:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217792_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 217792_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 247458_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 247458_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:11.50 +21:02:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.930 1826655019834242432 297.79878137358 +21.04253433258 12.0760 10.5242 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133524_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 133524_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 19381_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 19381_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 17730_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 17730_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 166890_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 166890_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 121200_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 121200_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 11451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 11451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 37680_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 37680_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 76615_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 76615_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 72674_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 72674_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 23129_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 23129_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 59912_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 59912_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 246980_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 246980_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:48:53.55 +20:07:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.790 1824992180293804160 297.22241974329 +20.11879173313 12.5348 10.3373 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213566_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 213566_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 67441_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 67441_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 103288_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 103288_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 131117_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 131117_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:04.00 +21:45:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78551_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 78551_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 44549_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 44549_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32962_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 32962_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 87874_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 87874_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 69649_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 69649_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 108249_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 108249_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:13.00 +20:52:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82733_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 82733_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 147316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 147316_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:32.76 +22:27:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.301 1827609842602409856 297.38524620816 +22.45817972356 11.8571 10.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92778_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 92778_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 75144_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 75144_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 46462_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 46462_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:14.26 +18:30:36.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)
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Considering the candidate 20982_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 20982_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 152128_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 152128_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:40:26.45 +23:05:26.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 206756_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 206756_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 232229_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 232229_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 36044_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 36044_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 131535_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 131535_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 86223_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 86223_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 136101_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 136101_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:05.42 +22:05:11.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 142738_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 142738_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 93629_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 93629_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 20948_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 20948_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 245789_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 245789_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:45.14 +19:44:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 0.431 1824778187845712128 297.68815868404 +19.74534649069 12.0924 10.5989 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116940_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 116940_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 97276_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 97276_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 114705_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 114705_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 175537_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 175537_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:16:35.83 +24:05:52.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 149736_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 149736_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:00.14 +22:51:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93016_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 93016_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:02:07.79 +20:30:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.750 1823713070310850560 300.53268077604 +20.51175223161 11.9021 10.2589 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 164451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 164451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 28532_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 28532_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 128220_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 128220_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 119088_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 119088_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 90998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 90998_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 94427_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 94427_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 47460_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 47460_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 170118_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 170118_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 103236_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 103236_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:34:28.98 +21:05:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 71371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:41:52.21 +19:54:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23939_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 23939_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 93562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 93562_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 193011_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 193011_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 65684_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 65684_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:39.67 +19:18:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 28941_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 28941_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 45675_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 45675_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 102997_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 102997_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:45:43.44 +20:37:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.591 1825826748314056576 296.43265826950 +20.62088762444 13.3507 12.4218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141706_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 141706_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 96374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 96374_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:41.98 +20:52:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83291_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 83291_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 60371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 60371_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:52:33.28 +19:06:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06814_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 06814_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:43:04.63 +17:05:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104779_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 104779_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 113453_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 113453_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 188075_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 188075_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 244971_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244971_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:32:12.39 +26:18:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.151 1856623897179813376 308.05223806852 +26.30759786019 12.0954 10.6424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244952_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244952_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:02.02 +19:57:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.476 1824973110635704832 296.75839594848 +19.95964583962 12.0931 10.4009 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 47511_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 47511_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:27.02 +18:29:40.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 244734_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 244734_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 244724_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244724_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 244685_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244685_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:50:33.64 +20:42:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 5.888 1814612210706521728 312.64150109099 +20.70413764000 11.7680 10.9760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244681_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244681_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:03:06.90 +18:48:49.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)
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Considering the candidate 169933_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 169933_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 19631_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 19631_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:00:32.69 +17:28:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.039 1820296410966078592 300.13706784927 +17.48053225764 13.4964 12.4651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 39678_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 39678_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 32495_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 32495_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:50.68 +17:51:14.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193325_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 193325_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 26365_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 26365_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 162520_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 162520_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 119293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 119293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 155969_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 155969_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 244533_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244533_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:47:03.89 +17:14:21.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
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Considering the candidate 244511_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244511_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:50.83 +18:57:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.115 1824587083326632448 296.96196213767 +18.95640945641 12.4534 11.0444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 244451_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 244449_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244449_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:16:07.64 +26:07:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.906 1835459672744543104 304.03257777536 +26.12417467116 11.0861 9.6196 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244432_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 244432_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 244328_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 244328_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:50:08.92 +19:52:41.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 40099_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 40099_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 179060_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 179060_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:56:51.50 +24:02:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.250 1834188564266763136 299.21495094981 +24.04982799882 12.0046 10.3839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28778_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 28778_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 65888_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 65888_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 127472_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 127472_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 13811_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 13811_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 94496_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 94496_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 219541_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 219541_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 34531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 34531_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:07:12.53 +18:12:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227200_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 227200_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 193018_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 193018_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 85751_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 85751_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 156293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 156293_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 243908_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 243908_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:16.85 +21:28:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.081 1826879118379509120 299.56968520176 +21.47337069180 12.4736 11.0153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243894_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 243894_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:00.04 +21:39:04.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)
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Considering the candidate 243812_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 243812_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:09:13.52 +17:38:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.622 1809850054063924480 302.30704029894 +17.63827483359 12.6052 11.1298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178547_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 178547_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 50058_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 50058_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:17.14 +18:40:06.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 11676_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 11676_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 111538_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 111538_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 243752_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 243752_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 243745_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 243745_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 224551_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 224551_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:53:48.40 +25:33:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59925_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 59925_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 40232_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 40232_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 180965_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 180965_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 192262_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 192262_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 82981_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 82981_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 174397_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 174397_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 150566_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 150566_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:21:32.08 +22:50:54.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 243413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 243413_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 220605_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 220605_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 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 127969_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 127969_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:11:21.22 +21:52:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 90279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 90279_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:27:14.17 +20:28:35.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 73668_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 73668_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:26:01.35 +19:51:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201455_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 201455_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:22:03.43 +24:26:41.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 92378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 92378_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:30:58.43 +20:36:23.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170224_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 170224_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:51:54.64 +23:29:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170260_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 170260_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 169134_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 169134_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 13634_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 13634_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:26:23.21 +17:18:56.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84304_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 84304_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 53611_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 53611_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:49:01.13 +18:45:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 16412_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:41:58.29 +17:31:18.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153976_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 153976_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:48:51.00 +22:59:37.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 177777_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 177777_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 20:38:31.78 +24:06:53.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77387_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 77387_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 48426_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 48426_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 170537_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 170537_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 64673_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
Preparing report for the candidate 64673_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
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Considering the candidate 47273_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 47273_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:54:54.94 +18:35:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74911_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 74911_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:58:45.96 +19:29:33.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54593_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227
The candidate 54593_fd_Vul-02-Q1b1x1_2026-04-09_03-47-22_20.00sec_-4.90C_LIGHTs_0227 did not pass the final checks
**** FOUND 19:47:23.84 +18:32:06.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 16s
make_report_in_HTML.sh TOTAL: 313s
Prepared the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:05:15.92 +17:40:53.4
20:04:21.94 +17:48:39.9
20:40:43.97 +18:56:32.8
20:24:31.54 +17:33:52.7
19:47:50.55 +17:51:15.5
19:51:56.44 +17:20:02.8
20:27:28.19 +24:17:20.6
20:02:28.78 +25:37:35.8
20:08:07.41 +18:46:14.8
19:47:34.74 +22:14:35.1
20:14:26.33 +17:05:17.5
20:09:50.96 +17:03:02.2
20:10:48.42 +17:08:59.0
19:52:42.12 +20:41:22.5
20:30:19.32 +21:06:49.1
20:11:37.52 +21:02:44.1
19:58:29.67 +20:53:09.5
20:13:22.85 +21:03:20.2
19:58:42.65 +20:54:21.1
20:03:14.54 +20:58:56.9
20:15:49.24 +21:07:56.2
20:00:44.84 +21:05:03.3
20:16:52.92 +21:20:21.2
20:22:16.04 +21:24:01.9
20:17:22.11 +21:22:41.6
20:01:00.99 +21:11:52.2
19:57:36.48 +21:11:04.8
20:05:47.38 +21:17:58.7
20:01:26.99 +21:15:51.6
20:05:42.68 +21:20:25.8
20:11:42.66 +17:12:40.1
19:47:14.17 +21:05:38.4
20:15:40.54 +21:31:15.9
19:59:36.58 +21:21:44.1
20:27:00.20 +17:20:14.8
20:06:22.34 +17:10:06.8
20:01:58.45 +21:25:01.4
20:04:36.23 +21:28:14.2
20:23:40.99 +17:17:39.1
20:07:12.87 +21:32:00.6
20:05:38.82 +21:32:33.3
19:49:05.44 +21:17:34.0
20:04:46.94 +21:35:49.5
20:02:57.04 +21:33:05.6
20:08:49.05 +21:40:22.9
19:50:14.56 +21:25:09.8
20:15:23.53 +21:45:01.1
20:15:47.96 +21:47:52.0
19:47:35.20 +21:24:58.4
20:11:01.54 +17:14:38.0
19:51:25.58 +21:29:31.4
20:16:59.05 +21:52:31.0
20:26:19.91 +21:56:40.5
20:11:42.55 +21:51:05.0
20:07:59.63 +21:53:59.1
19:58:35.62 +21:48:06.5
20:21:23.22 +22:01:46.3
20:06:40.13 +21:55:53.7
20:00:56.58 +21:55:32.7
20:14:59.13 +22:07:06.2
20:40:28.13 +22:13:09.4
20:00:41.51 +22:02:42.2
20:02:46.80 +22:04:59.4
20:50:19.98 +22:17:41.9
20:15:15.94 +22:17:16.9
20:31:40.28 +17:26:06.1
19:53:07.37 +22:01:46.0
19:59:05.59 +17:11:03.3
20:23:34.94 +22:27:34.5
20:15:37.93 +22:27:06.7
19:56:47.99 +22:19:39.1
19:52:21.45 +22:15:52.9
20:24:40.66 +22:39:03.7
20:04:27.32 +22:37:43.0
20:17:06.55 +22:45:42.7
19:50:42.88 +22:29:43.1
20:17:25.16 +17:25:58.8
20:24:15.28 +22:58:55.4
20:19:49.88 +17:26:05.2
20:17:28.95 +22:57:50.9
20:43:16.93 +23:01:32.0
20:01:50.06 +22:49:02.4
19:58:02.90 +22:49:27.2
20:27:11.28 +23:14:15.3
19:55:04.38 +22:55:52.9
19:55:13.67 +22:56:15.2
20:29:35.15 +23:15:55.1
19:52:37.20 +22:55:47.6
20:09:49.27 +17:24:16.9
20:45:06.34 +23:22:32.1
19:49:42.38 +22:58:05.5
19:55:53.02 +23:08:11.0
20:03:24.79 +23:19:49.9
20:49:30.70 +23:34:56.9
20:13:47.80 +23:32:49.4
20:21:49.11 +23:37:08.6
20:06:35.06 +23:31:20.9
20:08:20.29 +23:35:11.7
19:56:31.15 +23:26:10.2
20:43:02.35 +23:49:30.0
20:22:14.85 +23:48:13.0
20:47:44.13 +23:49:01.2
20:15:40.71 +23:47:45.6
19:52:56.70 +23:31:31.8
20:17:20.65 +23:50:18.4
20:01:09.13 +23:39:09.7
19:57:52.87 +23:37:26.2
20:50:57.44 +23:54:03.5
20:07:42.81 +23:54:51.9
20:02:58.53 +23:53:35.8
20:08:15.77 +23:58:00.7
19:53:51.32 +23:48:33.2
20:15:25.09 +24:10:03.7
20:44:30.33 +17:39:27.6
19:47:24.81 +23:50:31.0
20:30:41.06 +24:21:46.7
19:53:38.83 +24:05:57.7
20:03:45.07 +24:20:40.3
20:06:40.02 +25:01:29.2
20:37:17.17 +25:02:14.3
20:36:21.76 +24:58:36.7
20:13:31.14 +24:50:33.4
19:59:01.04 +24:41:25.0
20:24:02.63 +24:58:50.2
19:59:52.28 +24:38:51.2
20:00:35.84 +17:28:08.3
19:51:09.11 +24:27:56.2
20:14:05.43 +24:45:50.4
20:25:58.51 +24:48:41.8
20:14:56.46 +24:39:28.8
20:26:50.19 +24:43:12.7
20:01:30.29 +24:27:53.8
20:08:48.65 +24:30:26.5
20:24:38.37 +24:35:27.4
20:08:52.68 +24:28:02.6
20:21:30.30 +24:32:50.4
20:21:43.46 +26:53:41.8
19:58:06.44 +17:28:45.7
20:14:07.94 +17:40:56.6
20:08:07.32 +17:37:17.6
19:50:42.68 +17:24:25.0
20:14:35.27 +26:27:12.8
20:29:17.23 +26:17:26.5
20:31:12.49 +26:12:24.7
20:33:44.74 +26:03:25.1
20:00:54.89 +25:33:41.5
20:43:19.63 +25:45:32.0
20:29:15.90 +25:38:39.7
20:08:42.58 +17:43:52.8
20:35:42.16 +25:29:11.7
20:00:22.88 +17:40:17.3
20:11:51.46 +25:18:24.1
20:22:57.97 +22:38:12.4
20:02:16.65 +19:43:49.5
20:47:59.39 +18:18:46.3
20:44:14.72 +25:13:23.8
19:59:37.93 +22:44:01.4
20:23:38.98 +17:53:35.3
20:00:00.39 +17:41:20.4
19:48:54.38 +17:33:43.7
20:01:25.53 +17:44:55.4
20:24:21.49 +17:58:51.3
19:50:58.64 +17:38:58.1
20:37:21.60 +24:34:07.0
20:37:01.79 +17:33:04.4
20:15:04.38 +23:54:56.2
20:47:32.05 +20:43:38.9
20:10:08.48 +23:34:32.2
19:50:37.70 +21:28:40.0
20:28:04.24 +26:55:18.8
20:14:33.38 +23:02:32.8
20:16:41.67 +26:56:03.6
20:27:59.17 +19:58:15.2
20:12:33.13 +19:36:58.2
20:14:36.70 +23:14:36.6
20:29:10.53 +22:28:13.9
20:48:43.15 +18:50:39.7
20:12:14.11 +19:04:34.6
20:25:55.22 +25:47:16.2
20:33:16.98 +19:33:27.4
20:28:30.55 +18:22:09.4
20:41:41.30 +21:03:29.5
20:47:41.25 +17:08:04.0
19:58:26.46 +17:50:44.3
20:38:47.50 +20:11:01.1
20:52:31.78 +25:28:10.0
20:45:50.00 +22:19:09.2
20:04:11.49 +19:17:58.7
19:58:07.09 +22:16:03.0
20:49:50.88 +19:51:11.4
20:02:14.15 +17:48:58.6
20:19:34.22 +17:59:12.0
20:49:21.64 +19:35:34.8
19:48:12.58 +20:30:11.6
20:08:26.50 +25:35:49.5
20:06:06.80 +21:49:46.5
20:10:53.63 +17:55:01.9
20:36:34.35 +18:05:21.6
20:04:06.93 +17:51:13.9
20:08:02.30 +17:58:46.3
19:53:58.54 +17:48:12.2
20:06:24.32 +17:59:01.0
19:52:30.45 +17:51:19.2
20:10:37.48 +18:04:58.2
19:51:41.19 +17:53:36.6
20:03:51.57 +18:04:50.6
20:13:20.37 +18:11:32.2
20:32:01.45 +18:20:33.1
20:07:52.72 +18:13:35.3
20:12:24.55 +18:18:53.1
20:20:54.23 +18:21:22.8
20:32:04.56 +18:24:25.3
19:55:16.79 +18:07:45.3
20:19:02.63 +18:23:10.6
19:50:37.72 +18:05:40.8
20:43:37.45 +18:31:30.0
19:54:04.90 +18:11:17.9
20:04:26.41 +18:19:43.0
20:14:39.33 +18:26:56.8
19:51:37.84 +18:13:32.8
19:51:28.71 +18:15:18.4
20:08:47.24 +18:26:44.2
20:02:22.52 +18:23:49.3
19:57:42.24 +18:21:42.3
19:52:13.54 +18:20:10.4
19:53:48.78 +18:22:01.7
20:13:37.75 +18:40:11.8
20:30:37.66 +18:47:46.1
20:00:37.54 +18:34:16.2
20:00:21.53 +18:35:40.9
20:27:19.96 +18:49:58.7
19:59:47.11 +18:37:37.5
20:40:44.55 +18:56:26.6
20:14:09.78 +18:48:00.9
20:06:49.34 +18:43:43.3
20:01:35.38 +18:44:45.7
20:16:20.87 +18:55:29.1
20:25:53.94 +19:00:51.0
20:08:56.44 +18:58:02.8
20:20:31.49 +18:58:09.9
19:48:46.73 +18:44:48.9
20:25:00.19 +19:13:05.7
19:48:08.88 +18:51:21.4
19:46:45.29 +18:57:12.3
19:58:35.63 +19:10:06.4
20:03:31.36 +19:13:13.5
19:49:57.29 +19:02:38.5
20:08:11.55 +19:18:21.3
20:32:24.59 +19:29:38.6
20:17:50.60 +19:30:03.0
19:57:29.25 +19:17:29.0
19:53:45.53 +19:16:51.9
20:06:31.89 +19:27:39.3
20:01:07.73 +19:25:34.4
19:51:20.03 +19:18:23.3
19:46:30.71 +19:11:21.9
20:09:34.60 +19:32:28.4
20:01:12.90 +19:29:37.7
20:01:29.96 +19:31:49.9
20:04:12.73 +19:34:24.4
19:59:07.17 +19:34:09.3
20:32:28.67 +19:48:51.0
19:57:54.00 +19:33:34.2
20:14:51.36 +19:48:06.1
20:29:26.73 +19:53:18.7
20:25:45.09 +19:55:45.7
19:56:26.87 +19:38:44.8
20:04:44.14 +19:45:32.4
20:37:33.17 +20:03:17.4
19:47:09.52 +19:36:09.5
20:25:31.86 +20:03:07.8
20:49:18.71 +20:05:13.0
19:51:16.41 +19:44:57.1
20:20:57.86 +20:06:52.4
20:03:01.51 +19:57:20.6
19:55:05.05 +19:55:03.2
20:13:52.49 +20:09:59.7
20:34:33.56 +20:18:15.2
20:02:21.20 +20:05:14.6
20:48:11.43 +20:19:40.8
20:13:05.15 +20:14:32.6
20:24:30.66 +20:19:50.2
20:18:06.30 +20:17:16.1
19:57:35.40 +20:04:54.8
20:20:42.72 +20:18:49.8
20:02:13.53 +20:09:24.4
20:12:27.08 +20:16:49.3
20:49:47.34 +20:24:36.3
20:09:00.22 +20:18:27.6
20:33:54.20 +20:27:24.2
19:56:43.00 +20:09:57.2
20:36:00.54 +20:30:03.7
20:04:28.49 +20:18:28.5
20:06:34.15 +20:21:40.7
19:53:49.52 +20:17:54.6
20:32:06.82 +20:39:07.1
20:05:09.47 +20:31:30.8
20:15:31.03 +20:39:23.5
19:47:18.37 +20:18:06.6
19:55:21.50 +20:26:20.7
20:25:29.98 +20:44:57.3
20:26:04.45 +20:46:13.2
20:21:44.75 +20:47:34.1
20:33:48.60 +20:48:07.2
19:51:56.13 +20:31:52.2
20:12:01.84 +20:49:41.6
20:21:24.87 +20:54:36.1
20:34:00.58 +20:58:41.9
########### Completed Vul-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:24:31.54 +17:33:52.7
19:47:50.55 +17:51:15.5
19:51:56.44 +17:20:02.8
20:27:28.19 +24:17:20.6
20:02:28.78 +25:37:35.8
20:08:07.41 +18:46:14.8
19:47:34.74 +22:14:35.1
20:04:21.94 +17:48:39.9
20:05:15.92 +17:40:53.4
20:40:43.97 +18:56:32.8
20:37:21.60 +24:34:07.0
20:37:01.79 +17:33:04.4
20:15:04.38 +23:54:56.2
20:47:32.05 +20:43:38.9
20:10:08.48 +23:34:32.2
19:50:37.70 +21:28:40.0
20:28:04.24 +26:55:18.8
20:14:33.38 +23:02:32.8
20:16:41.67 +26:56:03.6
20:27:59.17 +19:58:15.2
20:12:33.13 +19:36:58.2
20:14:36.70 +23:14:36.6
20:29:10.53 +22:28:13.9
20:48:43.15 +18:50:39.7
20:12:14.11 +19:04:34.6
20:25:55.22 +25:47:16.2
20:33:16.98 +19:33:27.4
20:28:30.55 +18:22:09.4
20:41:41.30 +21:03:29.5
20:47:41.25 +17:08:04.0
19:58:26.46 +17:50:44.3
20:38:47.50 +20:11:01.1
20:52:31.78 +25:28:10.0
20:45:50.00 +22:19:09.2
20:04:11.49 +19:17:58.7
19:58:07.09 +22:16:03.0
20:49:50.88 +19:51:11.4
20:49:21.64 +19:35:34.8
19:48:12.58 +20:30:11.6
20:08:26.50 +25:35:49.5
20:06:06.80 +21:49:46.5
20:04:27.32 +22:37:43.0
19:57:42.24 +18:21:42.3
20:06:35.06 +23:31:20.9
19:58:35.62 +21:48:06.5
20:15:23.53 +21:45:01.1
20:43:37.45 +18:31:30.0
20:36:00.54 +20:30:03.7
20:43:16.93 +23:01:32.0
19:58:29.67 +20:53:09.5
19:53:48.78 +18:22:01.7
19:50:37.72 +18:05:40.8
19:49:42.38 +22:58:05.5
20:15:47.96 +21:47:52.0
20:15:31.03 +20:39:23.5
20:15:49.24 +21:07:56.2
19:53:07.37 +22:01:46.0
20:11:42.55 +21:51:05.0
20:05:47.38 +21:17:58.7
20:17:06.55 +22:45:42.7
19:57:54.00 +19:33:34.2
19:57:36.48 +21:11:04.8
19:55:16.79 +18:07:45.3
19:53:45.53 +19:16:51.9
20:20:31.49 +18:58:09.9
20:43:02.35 +23:49:30.0
20:13:47.80 +23:32:49.4
19:55:05.05 +19:55:03.2
20:04:36.23 +21:28:14.2
20:23:34.94 +22:27:34.5
20:04:12.73 +19:34:24.4
19:59:36.58 +21:21:44.1
20:50:19.98 +22:17:41.9
20:14:26.33 +17:05:17.5
20:21:30.30 +24:32:50.4
20:17:50.60 +19:30:03.0
19:51:09.11 +24:27:56.2
20:11:37.52 +21:02:44.1
19:51:20.03 +19:18:23.3
20:32:24.59 +19:29:38.6
20:30:37.66 +18:47:46.1
20:07:12.87 +21:32:00.6
20:21:24.87 +20:54:36.1
20:24:38.37 +24:35:27.4
20:09:34.60 +19:32:28.4
20:25:31.86 +20:03:07.8
20:08:11.55 +19:18:21.3
20:29:35.15 +23:15:55.1
20:20:57.86 +20:06:52.4
20:15:25.09 +24:10:03.7
20:02:22.52 +18:23:49.3
20:04:26.41 +18:19:43.0
20:17:28.95 +22:57:50.9
19:48:08.88 +18:51:21.4
19:58:35.63 +19:10:06.4
19:59:47.11 +18:37:37.5
20:21:49.11 +23:37:08.6
20:14:05.43 +24:45:50.4
20:49:47.34 +20:24:36.3
20:36:34.35 +18:05:21.6
20:06:49.34 +18:43:43.3
20:32:01.45 +18:20:33.1
20:26:50.19 +24:43:12.7
20:01:00.99 +21:11:52.2
20:07:52.72 +18:13:35.3
20:25:45.09 +19:55:45.7
20:14:39.33 +18:26:56.8
20:37:17.17 +25:02:14.3
20:04:46.94 +21:35:49.5
20:14:56.46 +24:39:28.8
19:53:49.52 +20:17:54.6
19:50:14.56 +21:25:09.8
19:48:54.38 +17:33:43.7
20:22:14.85 +23:48:13.0
20:03:14.54 +20:58:56.9
20:00:00.39 +17:41:20.4
20:11:01.54 +17:14:38.0
20:23:40.99 +17:17:39.1
20:19:34.22 +17:59:12.0
19:55:53.02 +23:08:11.0
20:16:52.92 +21:20:21.2
20:04:44.14 +19:45:32.4
20:16:20.87 +18:55:29.1
20:25:58.51 +24:48:41.8
20:04:28.49 +20:18:28.5
20:33:44.74 +26:03:25.1
20:18:06.30 +20:17:16.1
20:26:19.91 +21:56:40.5
20:03:45.07 +24:20:40.3
20:13:37.75 +18:40:11.8
20:00:44.84 +21:05:03.3
20:15:15.94 +22:17:16.9
20:01:25.53 +17:44:55.4
20:24:21.49 +17:58:51.3
20:01:50.06 +22:49:02.4
19:52:37.20 +22:55:47.6
20:31:40.28 +17:26:06.1
19:52:42.12 +20:41:22.5
20:06:40.13 +21:55:53.7
20:34:00.58 +20:58:41.9
19:55:13.67 +22:56:15.2
20:13:52.49 +20:09:59.7
19:57:29.25 +19:17:29.0
20:29:15.90 +25:38:39.7
19:52:13.54 +18:20:10.4
19:52:30.45 +17:51:19.2
20:45:06.34 +23:22:32.1
20:40:44.55 +18:56:26.6
20:14:59.13 +22:07:06.2
19:51:41.19 +17:53:36.6
20:09:50.96 +17:03:02.2
20:13:20.37 +18:11:32.2
20:25:00.19 +19:13:05.7
20:24:15.28 +22:58:55.4
20:06:24.32 +17:59:01.0
20:19:02.63 +18:23:10.6
20:08:56.44 +18:58:02.8
20:05:42.68 +21:20:25.8
20:02:13.53 +20:09:24.4
20:30:41.06 +24:21:46.7
19:57:35.40 +20:04:54.8
20:00:56.58 +21:55:32.7
19:46:45.29 +18:57:12.3
19:53:51.32 +23:48:33.2
20:16:59.05 +21:52:31.0
20:50:57.44 +23:54:03.5
20:13:31.14 +24:50:33.4
20:08:15.77 +23:58:00.7
20:15:40.54 +21:31:15.9
20:25:53.94 +19:00:51.0
20:14:51.36 +19:48:06.1
19:50:42.68 +17:24:25.0
20:08:20.29 +23:35:11.7
19:58:02.90 +22:49:27.2
19:58:06.44 +17:28:45.7
20:20:54.23 +18:21:22.8
20:29:26.73 +19:53:18.7
19:56:47.99 +22:19:39.1
20:10:37.48 +18:04:58.2
20:19:49.88 +17:26:05.2
20:20:42.72 +20:18:49.8
20:33:54.20 +20:27:24.2
20:10:53.63 +17:55:01.9
20:12:01.84 +20:49:41.6
19:47:35.20 +21:24:58.4
20:27:00.20 +17:20:14.8
20:08:52.68 +24:28:02.6
20:01:29.96 +19:31:49.9
20:00:02.88 +22:46:48.2
20:02:46.80 +22:04:59.4
19:58:42.65 +20:54:21.1
19:51:25.58 +21:29:31.4
20:17:22.11 +21:22:41.6
20:09:49.27 +17:24:16.9
20:08:49.05 +21:40:22.9
20:43:19.63 +25:45:32.0
20:21:44.75 +20:47:34.1
20:34:33.56 +20:18:15.2
20:07:42.81 +23:54:51.9
20:01:07.73 +19:25:34.4
19:50:42.88 +22:29:43.1
20:02:21.20 +20:05:14.6
19:48:46.73 +18:44:48.9
20:15:37.93 +22:27:06.7
20:17:25.16 +17:25:58.8
19:51:56.13 +20:31:52.2
20:12:24.55 +18:18:53.1
19:47:09.52 +19:36:09.5
20:01:30.29 +24:27:53.8
20:23:38.98 +17:53:35.3
20:00:21.53 +18:35:40.9
20:01:09.13 +23:39:09.7
20:32:28.67 +19:48:51.0
20:10:48.42 +17:08:59.0
20:02:14.15 +17:48:58.6
20:08:48.65 +24:30:26.5
20:29:17.23 +26:17:26.5
20:00:41.51 +22:02:42.2
20:00:35.84 +17:28:08.3
20:44:30.33 +17:39:27.6
19:56:31.15 +23:26:10.2
20:02:57.04 +21:33:05.6
20:11:42.66 +17:12:40.1
19:54:04.90 +18:11:17.9
20:49:18.71 +20:05:13.0
19:56:26.87 +19:38:44.8
20:08:42.58 +17:43:52.8
20:03:31.36 +19:13:13.5
20:14:35.27 +26:27:12.8
20:01:12.90 +19:29:37.7
20:30:19.32 +21:06:49.1
20:03:01.51 +19:57:20.6
20:00:37.54 +18:34:16.2
20:03:51.57 +18:04:50.6
20:06:34.15 +20:21:40.7
19:59:07.17 +19:34:09.3
20:48:11.43 +20:19:40.8
20:05:09.47 +20:31:30.8
20:37:33.17 +20:03:17.4
20:08:07.32 +17:37:17.6
20:21:43.46 +26:53:41.8
20:35:42.16 +25:29:11.7
20:32:04.56 +18:24:25.3
20:40:28.13 +22:13:09.4
19:56:43.00 +20:09:57.2
20:24:40.66 +22:39:03.7
19:55:21.50 +20:26:20.7
20:14:07.94 +17:40:56.6
20:01:58.45 +21:25:01.4
20:33:48.60 +20:48:07.2
19:47:14.17 +21:05:38.4
20:49:30.70 +23:34:56.9
20:04:06.93 +17:51:13.9
20:21:23.22 +22:01:46.3
20:05:38.82 +21:32:33.3
20:32:06.82 +20:39:07.1
20:25:29.98 +20:44:57.3
20:14:09.78 +18:48:00.9
19:52:56.70 +23:31:31.8
20:00:22.88 +17:40:17.3
19:47:18.37 +20:18:06.6
19:59:01.04 +24:41:25.0
19:53:58.54 +17:48:12.2
20:27:19.96 +18:49:58.7
19:52:21.45 +22:15:52.9
20:24:30.66 +20:19:50.2
20:13:22.85 +21:03:20.2
20:01:26.99 +21:15:51.6
20:06:40.02 +25:01:29.2
19:59:37.93 +22:44:01.4
20:15:40.71 +23:47:45.6
19:51:37.84 +18:13:32.8
19:59:52.28 +24:38:51.2
19:50:58.64 +17:38:58.1
20:03:24.79 +23:19:49.9
19:49:05.44 +21:17:34.0
20:27:11.28 +23:14:15.3
20:44:14.72 +25:13:23.8
20:47:59.39 +18:18:46.3
19:51:28.71 +18:15:18.4
20:08:02.30 +17:58:46.3
19:46:30.71 +19:11:21.9
20:07:59.63 +21:53:59.1
19:59:05.59 +17:11:03.3
20:26:04.45 +20:46:13.2
20:31:12.49 +26:12:24.7
20:00:54.89 +25:33:41.5
20:24:02.63 +24:58:50.2
20:09:00.22 +20:18:27.6
19:55:04.38 +22:55:52.9
19:47:24.81 +23:50:31.0
20:06:22.34 +17:10:06.8
20:22:16.04 +21:24:01.9
20:02:16.65 +19:43:49.5
20:22:57.97 +22:38:12.4
19:49:57.29 +19:02:38.5
20:08:47.24 +18:26:44.2
19:53:38.83 +24:05:57.7
20:36:21.76 +24:58:36.7
20:13:05.15 +20:14:32.6
20:02:58.53 +23:53:35.8
20:11:51.46 +25:18:24.1
20:17:20.65 +23:50:18.4
20:47:44.13 +23:49:01.2
20:12:27.08 +20:16:49.3
19:51:16.41 +19:44:57.1
20:01:35.38 +18:44:45.7
19:57:52.87 +23:37:26.2
20:06:31.89 +19:27:39.3
###################################################################################
20:24:31.54 +17:33:52.7 -- not an asteroid (will add it to exclusion list)
19:47:50.55 +17:51:15.5 -- not an asteroid (will add it to exclusion list)
19:51:56.44 +17:20:02.8 -- not an asteroid (will add it to exclusion list)
20:27:28.19 +24:17:20.6 -- not an asteroid (will add it to exclusion list)
20:02:28.78 +25:37:35.8 -- not an asteroid (will add it to exclusion list)
20:08:07.41 +18:46:14.8 -- not an asteroid (will add it to exclusion list)
19:47:34.74 +22:14:35.1 -- not an asteroid (will add it to exclusion list)
20:04:21.94 +17:48:39.9 -- not an asteroid (will add it to exclusion list)
20:05:15.92 +17:40:53.4 -- not an asteroid (will add it to exclusion list)
20:40:43.97 +18:56:32.8 -- not an asteroid (will add it to exclusion list)
20:37:21.60 +24:34:07.0 -- not an asteroid (will add it to exclusion list)
20:37:01.79 +17:33:04.4 -- not an asteroid (will add it to exclusion list)
20:15:04.38 +23:54:56.2 -- not an asteroid (will add it to exclusion list)
20:47:32.05 +20:43:38.9 -- not an asteroid (will add it to exclusion list)
20:10:08.48 +23:34:32.2 -- not an asteroid (will add it to exclusion list)
19:50:37.70 +21:28:40.0 -- not an asteroid (will add it to exclusion list)
20:28:04.24 +26:55:18.8 -- not an asteroid (will add it to exclusion list)
20:14:33.38 +23:02:32.8 -- not an asteroid (will add it to exclusion list)
20:16:41.67 +26:56:03.6 -- not an asteroid (will add it to exclusion list)
20:27:59.17 +19:58:15.2 -- not an asteroid (will add it to exclusion list)
20:12:33.13 +19:36:58.2 -- not an asteroid (will add it to exclusion list)
20:14:36.70 +23:14:36.6 -- not an asteroid (will add it to exclusion list)
20:29:10.53 +22:28:13.9 -- not an asteroid (will add it to exclusion list)
20:48:43.15 +18:50:39.7 -- not an asteroid (will add it to exclusion list)
20:12:14.11 +19:04:34.6 -- not an asteroid (will add it to exclusion list)
20:25:55.22 +25:47:16.2 -- not an asteroid (will add it to exclusion list)
20:33:16.98 +19:33:27.4 -- not an asteroid (will add it to exclusion list)
20:28:30.55 +18:22:09.4 -- not an asteroid (will add it to exclusion list)
20:41:41.30 +21:03:29.5 -- not an asteroid (will add it to exclusion list)
20:47:41.25 +17:08:04.0 -- not an asteroid (will add it to exclusion list)
19:58:26.46 +17:50:44.3 -- not an asteroid (will add it to exclusion list)
20:38:47.50 +20:11:01.1 -- not an asteroid (will add it to exclusion list)
20:52:31.78 +25:28:10.0 -- not an asteroid (will add it to exclusion list)
20:45:50.00 +22:19:09.2 -- not an asteroid (will add it to exclusion list)
20:04:11.49 +19:17:58.7 -- not an asteroid (will add it to exclusion list)
19:58:07.09 +22:16:03.0 -- not an asteroid (will add it to exclusion list)
20:49:50.88 +19:51:11.4 -- not an asteroid (will add it to exclusion list)
20:49:21.64 +19:35:34.8 -- not an asteroid (will add it to exclusion list)
19:48:12.58 +20:30:11.6 -- not an asteroid (will add it to exclusion list)
20:08:26.50 +25:35:49.5 -- not an asteroid (will add it to exclusion list)
20:06:06.80 +21:49:46.5 -- not an asteroid (will add it to exclusion list)
20:04:27.32 +22:37:43.0 -- not an asteroid (will add it to exclusion list)
19:57:42.24 +18:21:42.3 -- not an asteroid (will add it to exclusion list)
20:06:35.06 +23:31:20.9 -- not an asteroid (will add it to exclusion list)
19:58:35.62 +21:48:06.5 -- not an asteroid (will add it to exclusion list)
20:15:23.53 +21:45:01.1 -- not an asteroid (will add it to exclusion list)
20:43:37.45 +18:31:30.0 -- not an asteroid (will add it to exclusion list)
20:36:00.54 +20:30:03.7 -- not an asteroid (will add it to exclusion list)
20:43:16.93 +23:01:32.0 -- not an asteroid (will add it to exclusion list)
19:58:29.67 +20:53:09.5 -- not an asteroid (will add it to exclusion list)
19:53:48.78 +18:22:01.7 -- not an asteroid (will add it to exclusion list)
19:50:37.72 +18:05:40.8 -- not an asteroid (will add it to exclusion list)
19:49:42.38 +22:58:05.5 -- not an asteroid (will add it to exclusion list)
20:15:47.96 +21:47:52.0 -- not an asteroid (will add it to exclusion list)
20:15:31.03 +20:39:23.5 -- not an asteroid (will add it to exclusion list)
20:15:49.24 +21:07:56.2 -- not an asteroid (will add it to exclusion list)
19:53:07.37 +22:01:46.0 -- not an asteroid (will add it to exclusion list)
20:11:42.55 +21:51:05.0 -- not an asteroid (will add it to exclusion list)
20:05:47.38 +21:17:58.7 -- not an asteroid (will add it to exclusion list)
20:17:06.55 +22:45:42.7 -- not an asteroid (will add it to exclusion list)
19:57:54.00 +19:33:34.2 -- not an asteroid (will add it to exclusion list)
19:57:36.48 +21:11:04.8 -- not an asteroid (will add it to exclusion list)
19:55:16.79 +18:07:45.3 -- not an asteroid (will add it to exclusion list)
19:53:45.53 +19:16:51.9 -- not an asteroid (will add it to exclusion list)
20:20:31.49 +18:58:09.9 -- not an asteroid (will add it to exclusion list)
20:43:02.35 +23:49:30.0 -- not an asteroid (will add it to exclusion list)
20:13:47.80 +23:32:49.4 -- not an asteroid (will add it to exclusion list)
19:55:05.05 +19:55:03.2 -- not an asteroid (will add it to exclusion list)
20:04:36.23 +21:28:14.2 -- not an asteroid (will add it to exclusion list)
20:23:34.94 +22:27:34.5 -- not an asteroid (will add it to exclusion list)
20:04:12.73 +19:34:24.4 -- not an asteroid (will add it to exclusion list)
19:59:36.58 +21:21:44.1 -- not an asteroid (will add it to exclusion list)
20:50:19.98 +22:17:41.9 -- not an asteroid (will add it to exclusion list)
20:14:26.33 +17:05:17.5 -- not an asteroid (will add it to exclusion list)
20:21:30.30 +24:32:50.4 -- not an asteroid (will add it to exclusion list)
20:17:50.60 +19:30:03.0 -- not an asteroid (will add it to exclusion list)
19:51:09.11 +24:27:56.2 -- not an asteroid (will add it to exclusion list)
20:11:37.52 +21:02:44.1 -- not an asteroid (will add it to exclusion list)
19:51:20.03 +19:18:23.3 -- not an asteroid (will add it to exclusion list)
20:32:24.59 +19:29:38.6 -- not an asteroid (will add it to exclusion list)
20:30:37.66 +18:47:46.1 -- not an asteroid (will add it to exclusion list)
20:07:12.87 +21:32:00.6 -- not an asteroid (will add it to exclusion list)
20:21:24.87 +20:54:36.1 -- not an asteroid (will add it to exclusion list)
20:24:38.37 +24:35:27.4 -- not an asteroid (will add it to exclusion list)
20:09:34.60 +19:32:28.4 -- not an asteroid (will add it to exclusion list)
20:25:31.86 +20:03:07.8 -- not an asteroid (will add it to exclusion list)
20:08:11.55 +19:18:21.3 -- not an asteroid (will add it to exclusion list)
20:29:35.15 +23:15:55.1 -- not an asteroid (will add it to exclusion list)
20:20:57.86 +20:06:52.4 -- not an asteroid (will add it to exclusion list)
20:15:25.09 +24:10:03.7 -- not an asteroid (will add it to exclusion list)
20:02:22.52 +18:23:49.3 -- not an asteroid (will add it to exclusion list)
20:04:26.41 +18:19:43.0 -- not an asteroid (will add it to exclusion list)
20:17:28.95 +22:57:50.9 -- not an asteroid (will add it to exclusion list)
19:48:08.88 +18:51:21.4 -- not an asteroid (will add it to exclusion list)
19:58:35.63 +19:10:06.4 -- not an asteroid (will add it to exclusion list)
19:59:47.11 +18:37:37.5 -- not an asteroid (will add it to exclusion list)
20:21:49.11 +23:37:08.6 -- not an asteroid (will add it to exclusion list)
20:14:05.43 +24:45:50.4 -- not an asteroid (will add it to exclusion list)
20:49:47.34 +20:24:36.3 -- not an asteroid (will add it to exclusion list)
20:36:34.35 +18:05:21.6 -- not an asteroid (will add it to exclusion list)
20:06:49.34 +18:43:43.3 -- not an asteroid (will add it to exclusion list)
20:32:01.45 +18:20:33.1 -- not an asteroid (will add it to exclusion list)
20:26:50.19 +24:43:12.7 -- not an asteroid (will add it to exclusion list)
20:01:00.99 +21:11:52.2 -- not an asteroid (will add it to exclusion list)
20:07:52.72 +18:13:35.3 -- not an asteroid (will add it to exclusion list)
20:25:45.09 +19:55:45.7 -- not an asteroid (will add it to exclusion list)
20:14:39.33 +18:26:56.8 -- not an asteroid (will add it to exclusion list)
20:37:17.17 +25:02:14.3 -- not an asteroid (will add it to exclusion list)
20:04:46.94 +21:35:49.5 -- not an asteroid (will add it to exclusion list)
20:14:56.46 +24:39:28.8 -- not an asteroid (will add it to exclusion list)
19:53:49.52 +20:17:54.6 -- not an asteroid (will add it to exclusion list)
19:50:14.56 +21:25:09.8 -- not an asteroid (will add it to exclusion list)
19:48:54.38 +17:33:43.7 -- not an asteroid (will add it to exclusion list)
20:22:14.85 +23:48:13.0 -- not an asteroid (will add it to exclusion list)
20:03:14.54 +20:58:56.9 -- not an asteroid (will add it to exclusion list)
20:00:00.39 +17:41:20.4 -- not an asteroid (will add it to exclusion list)
20:11:01.54 +17:14:38.0 -- not an asteroid (will add it to exclusion list)
20:23:40.99 +17:17:39.1 -- not an asteroid (will add it to exclusion list)
20:19:34.22 +17:59:12.0 -- not an asteroid (will add it to exclusion list)
19:55:53.02 +23:08:11.0 -- not an asteroid (will add it to exclusion list)
20:16:52.92 +21:20:21.2 -- not an asteroid (will add it to exclusion list)
20:04:44.14 +19:45:32.4 -- not an asteroid (will add it to exclusion list)
20:16:20.87 +18:55:29.1 -- not an asteroid (will add it to exclusion list)
20:25:58.51 +24:48:41.8 -- not an asteroid (will add it to exclusion list)
20:04:28.49 +20:18:28.5 -- not an asteroid (will add it to exclusion list)
20:33:44.74 +26:03:25.1 -- not an asteroid (will add it to exclusion list)
20:18:06.30 +20:17:16.1 -- not an asteroid (will add it to exclusion list)
20:26:19.91 +21:56:40.5 -- not an asteroid (will add it to exclusion list)
20:03:45.07 +24:20:40.3 -- not an asteroid (will add it to exclusion list)
20:13:37.75 +18:40:11.8 -- not an asteroid (will add it to exclusion list)
20:00:44.84 +21:05:03.3 -- not an asteroid (will add it to exclusion list)
20:15:15.94 +22:17:16.9 -- not an asteroid (will add it to exclusion list)
20:01:25.53 +17:44:55.4 -- not an asteroid (will add it to exclusion list)
20:24:21.49 +17:58:51.3 -- not an asteroid (will add it to exclusion list)
20:01:50.06 +22:49:02.4 -- not an asteroid (will add it to exclusion list)
19:52:37.20 +22:55:47.6 -- not an asteroid (will add it to exclusion list)
20:31:40.28 +17:26:06.1 -- not an asteroid (will add it to exclusion list)
19:52:42.12 +20:41:22.5 -- not an asteroid (will add it to exclusion list)
20:06:40.13 +21:55:53.7 -- not an asteroid (will add it to exclusion list)
20:34:00.58 +20:58:41.9 -- not an asteroid (will add it to exclusion list)
19:55:13.67 +22:56:15.2 -- not an asteroid (will add it to exclusion list)
20:13:52.49 +20:09:59.7 -- not an asteroid (will add it to exclusion list)
19:57:29.25 +19:17:29.0 -- not an asteroid (will add it to exclusion list)
20:29:15.90 +25:38:39.7 -- not an asteroid (will add it to exclusion list)
19:52:13.54 +18:20:10.4 -- not an asteroid (will add it to exclusion list)
19:52:30.45 +17:51:19.2 -- not an asteroid (will add it to exclusion list)
20:45:06.34 +23:22:32.1 -- not an asteroid (will add it to exclusion list)
20:40:44.55 +18:56:26.6 -- not an asteroid (will add it to exclusion list)
20:14:59.13 +22:07:06.2 -- not an asteroid (will add it to exclusion list)
19:51:41.19 +17:53:36.6 -- not an asteroid (will add it to exclusion list)
20:09:50.96 +17:03:02.2 -- not an asteroid (will add it to exclusion list)
20:13:20.37 +18:11:32.2 -- not an asteroid (will add it to exclusion list)
20:25:00.19 +19:13:05.7 -- not an asteroid (will add it to exclusion list)
20:24:15.28 +22:58:55.4 -- not an asteroid (will add it to exclusion list)
20:06:24.32 +17:59:01.0 -- not an asteroid (will add it to exclusion list)
20:19:02.63 +18:23:10.6 -- not an asteroid (will add it to exclusion list)
20:08:56.44 +18:58:02.8 -- not an asteroid (will add it to exclusion list)
20:05:42.68 +21:20:25.8 -- not an asteroid (will add it to exclusion list)
20:02:13.53 +20:09:24.4 -- not an asteroid (will add it to exclusion list)
20:30:41.06 +24:21:46.7 -- not an asteroid (will add it to exclusion list)
19:57:35.40 +20:04:54.8 -- not an asteroid (will add it to exclusion list)
20:00:56.58 +21:55:32.7 -- not an asteroid (will add it to exclusion list)
19:46:45.29 +18:57:12.3 -- not an asteroid (will add it to exclusion list)
19:53:51.32 +23:48:33.2 -- not an asteroid (will add it to exclusion list)
20:16:59.05 +21:52:31.0 -- not an asteroid (will add it to exclusion list)
20:50:57.44 +23:54:03.5 -- not an asteroid (will add it to exclusion list)
20:13:31.14 +24:50:33.4 -- not an asteroid (will add it to exclusion list)
20:08:15.77 +23:58:00.7 -- not an asteroid (will add it to exclusion list)
20:15:40.54 +21:31:15.9 -- not an asteroid (will add it to exclusion list)
20:25:53.94 +19:00:51.0 -- not an asteroid (will add it to exclusion list)
20:14:51.36 +19:48:06.1 -- not an asteroid (will add it to exclusion list)
19:50:42.68 +17:24:25.0 -- not an asteroid (will add it to exclusion list)
20:08:20.29 +23:35:11.7 -- not an asteroid (will add it to exclusion list)
19:58:02.90 +22:49:27.2 -- not an asteroid (will add it to exclusion list)
19:58:06.44 +17:28:45.7 -- not an asteroid (will add it to exclusion list)
20:20:54.23 +18:21:22.8 -- not an asteroid (will add it to exclusion list)
20:29:26.73 +19:53:18.7 -- not an asteroid (will add it to exclusion list)
19:56:47.99 +22:19:39.1 -- not an asteroid (will add it to exclusion list)
20:10:37.48 +18:04:58.2 -- not an asteroid (will add it to exclusion list)
20:19:49.88 +17:26:05.2 -- not an asteroid (will add it to exclusion list)
20:20:42.72 +20:18:49.8 -- not an asteroid (will add it to exclusion list)
20:33:54.20 +20:27:24.2 -- not an asteroid (will add it to exclusion list)
20:10:53.63 +17:55:01.9 -- not an asteroid (will add it to exclusion list)
20:12:01.84 +20:49:41.6 -- not an asteroid (will add it to exclusion list)
19:47:35.20 +21:24:58.4 -- not an asteroid (will add it to exclusion list)
20:27:00.20 +17:20:14.8 -- not an asteroid (will add it to exclusion list)
20:08:52.68 +24:28:02.6 -- not an asteroid (will add it to exclusion list)
20:01:29.96 +19:31:49.9 -- not an asteroid (will add it to exclusion list)
20:00:02.88 +22:46:48.2 -- not an asteroid (will add it to exclusion list)
20:02:46.80 +22:04:59.4 -- not an asteroid (will add it to exclusion list)
19:58:42.65 +20:54:21.1 -- not an asteroid (will add it to exclusion list)
19:51:25.58 +21:29:31.4 -- not an asteroid (will add it to exclusion list)
20:17:22.11 +21:22:41.6 -- not an asteroid (will add it to exclusion list)
20:09:49.27 +17:24:16.9 -- not an asteroid (will add it to exclusion list)
20:08:49.05 +21:40:22.9 -- not an asteroid (will add it to exclusion list)
20:43:19.63 +25:45:32.0 -- not an asteroid (will add it to exclusion list)
20:21:44.75 +20:47:34.1 -- not an asteroid (will add it to exclusion list)
20:34:33.56 +20:18:15.2 -- not an asteroid (will add it to exclusion list)
20:07:42.81 +23:54:51.9 -- not an asteroid (will add it to exclusion list)
20:01:07.73 +19:25:34.4 -- not an asteroid (will add it to exclusion list)
19:50:42.88 +22:29:43.1 -- not an asteroid (will add it to exclusion list)
20:02:21.20 +20:05:14.6 -- not an asteroid (will add it to exclusion list)
19:48:46.73 +18:44:48.9 -- not an asteroid (will add it to exclusion list)
20:15:37.93 +22:27:06.7 -- not an asteroid (will add it to exclusion list)
20:17:25.16 +17:25:58.8 -- not an asteroid (will add it to exclusion list)
19:51:56.13 +20:31:52.2 -- not an asteroid (will add it to exclusion list)
20:12:24.55 +18:18:53.1 -- not an asteroid (will add it to exclusion list)
19:47:09.52 +19:36:09.5 -- not an asteroid (will add it to exclusion list)
20:01:30.29 +24:27:53.8 -- not an asteroid (will add it to exclusion list)
20:23:38.98 +17:53:35.3 -- not an asteroid (will add it to exclusion list)
20:00:21.53 +18:35:40.9 -- not an asteroid (will add it to exclusion list)
20:01:09.13 +23:39:09.7 -- not an asteroid (will add it to exclusion list)
20:32:28.67 +19:48:51.0 -- not an asteroid (will add it to exclusion list)
20:10:48.42 +17:08:59.0 -- not an asteroid (will add it to exclusion list)
20:02:14.15 +17:48:58.6 -- not an asteroid (will add it to exclusion list)
20:08:48.65 +24:30:26.5 -- not an asteroid (will add it to exclusion list)
20:29:17.23 +26:17:26.5 -- not an asteroid (will add it to exclusion list)
20:00:41.51 +22:02:42.2 -- not an asteroid (will add it to exclusion list)
20:00:35.84 +17:28:08.3 -- not an asteroid (will add it to exclusion list)
20:44:30.33 +17:39:27.6 -- not an asteroid (will add it to exclusion list)
19:56:31.15 +23:26:10.2 -- not an asteroid (will add it to exclusion list)
20:02:57.04 +21:33:05.6 -- not an asteroid (will add it to exclusion list)
20:11:42.66 +17:12:40.1 -- not an asteroid (will add it to exclusion list)
19:54:04.90 +18:11:17.9 -- not an asteroid (will add it to exclusion list)
20:49:18.71 +20:05:13.0 -- not an asteroid (will add it to exclusion list)
19:56:26.87 +19:38:44.8 -- not an asteroid (will add it to exclusion list)
20:08:42.58 +17:43:52.8 -- not an asteroid (will add it to exclusion list)
20:03:31.36 +19:13:13.5 -- not an asteroid (will add it to exclusion list)
20:14:35.27 +26:27:12.8 -- not an asteroid (will add it to exclusion list)
20:01:12.90 +19:29:37.7 -- not an asteroid (will add it to exclusion list)
20:30:19.32 +21:06:49.1 -- not an asteroid (will add it to exclusion list)
20:03:01.51 +19:57:20.6 -- not an asteroid (will add it to exclusion list)
20:00:37.54 +18:34:16.2 -- not an asteroid (will add it to exclusion list)
20:03:51.57 +18:04:50.6 -- not an asteroid (will add it to exclusion list)
20:06:34.15 +20:21:40.7 -- not an asteroid (will add it to exclusion list)
19:59:07.17 +19:34:09.3 -- not an asteroid (will add it to exclusion list)
20:48:11.43 +20:19:40.8 -- not an asteroid (will add it to exclusion list)
20:05:09.47 +20:31:30.8 -- not an asteroid (will add it to exclusion list)
20:37:33.17 +20:03:17.4 -- not an asteroid (will add it to exclusion list)
20:08:07.32 +17:37:17.6 -- not an asteroid (will add it to exclusion list)
20:21:43.46 +26:53:41.8 -- not an asteroid (will add it to exclusion list)
20:35:42.16 +25:29:11.7 -- not an asteroid (will add it to exclusion list)
20:32:04.56 +18:24:25.3 -- not an asteroid (will add it to exclusion list)
20:40:28.13 +22:13:09.4 -- not an asteroid (will add it to exclusion list)
19:56:43.00 +20:09:57.2 -- not an asteroid (will add it to exclusion list)
20:24:40.66 +22:39:03.7 -- not an asteroid (will add it to exclusion list)
19:55:21.50 +20:26:20.7 -- not an asteroid (will add it to exclusion list)
20:14:07.94 +17:40:56.6 -- not an asteroid (will add it to exclusion list)
20:01:58.45 +21:25:01.4 -- not an asteroid (will add it to exclusion list)
20:33:48.60 +20:48:07.2 -- not an asteroid (will add it to exclusion list)
19:47:14.17 +21:05:38.4 -- not an asteroid (will add it to exclusion list)
20:49:30.70 +23:34:56.9 -- not an asteroid (will add it to exclusion list)
20:04:06.93 +17:51:13.9 -- not an asteroid (will add it to exclusion list)
20:21:23.22 +22:01:46.3 -- not an asteroid (will add it to exclusion list)
20:05:38.82 +21:32:33.3 -- not an asteroid (will add it to exclusion list)
20:32:06.82 +20:39:07.1 -- not an asteroid (will add it to exclusion list)
20:25:29.98 +20:44:57.3 -- not an asteroid (will add it to exclusion list)
20:14:09.78 +18:48:00.9 -- not an asteroid (will add it to exclusion list)
19:52:56.70 +23:31:31.8 -- not an asteroid (will add it to exclusion list)
20:00:22.88 +17:40:17.3 -- not an asteroid (will add it to exclusion list)
19:47:18.37 +20:18:06.6 -- not an asteroid (will add it to exclusion list)
19:59:01.04 +24:41:25.0 -- not an asteroid (will add it to exclusion list)
19:53:58.54 +17:48:12.2 -- not an asteroid (will add it to exclusion list)
20:27:19.96 +18:49:58.7 -- not an asteroid (will add it to exclusion list)
19:52:21.45 +22:15:52.9 -- not an asteroid (will add it to exclusion list)
20:24:30.66 +20:19:50.2 -- not an asteroid (will add it to exclusion list)
20:13:22.85 +21:03:20.2 -- not an asteroid (will add it to exclusion list)
20:01:26.99 +21:15:51.6 -- not an asteroid (will add it to exclusion list)
20:06:40.02 +25:01:29.2 -- not an asteroid (will add it to exclusion list)
19:59:37.93 +22:44:01.4 -- not an asteroid (will add it to exclusion list)
20:15:40.71 +23:47:45.6 -- not an asteroid (will add it to exclusion list)
19:51:37.84 +18:13:32.8 -- not an asteroid (will add it to exclusion list)
19:59:52.28 +24:38:51.2 -- not an asteroid (will add it to exclusion list)
19:50:58.64 +17:38:58.1 -- not an asteroid (will add it to exclusion list)
20:03:24.79 +23:19:49.9 -- not an asteroid (will add it to exclusion list)
19:49:05.44 +21:17:34.0 -- not an asteroid (will add it to exclusion list)
20:27:11.28 +23:14:15.3 -- not an asteroid (will add it to exclusion list)
20:44:14.72 +25:13:23.8 -- not an asteroid (will add it to exclusion list)
20:47:59.39 +18:18:46.3 -- not an asteroid (will add it to exclusion list)
19:51:28.71 +18:15:18.4 -- not an asteroid (will add it to exclusion list)
20:08:02.30 +17:58:46.3 -- not an asteroid (will add it to exclusion list)
19:46:30.71 +19:11:21.9 -- not an asteroid (will add it to exclusion list)
20:07:59.63 +21:53:59.1 -- not an asteroid (will add it to exclusion list)
19:59:05.59 +17:11:03.3 -- not an asteroid (will add it to exclusion list)
20:26:04.45 +20:46:13.2 -- not an asteroid (will add it to exclusion list)
20:31:12.49 +26:12:24.7 -- not an asteroid (will add it to exclusion list)
20:00:54.89 +25:33:41.5 -- not an asteroid (will add it to exclusion list)
20:24:02.63 +24:58:50.2 -- not an asteroid (will add it to exclusion list)
20:09:00.22 +20:18:27.6 -- not an asteroid (will add it to exclusion list)
19:55:04.38 +22:55:52.9 -- not an asteroid (will add it to exclusion list)
19:47:24.81 +23:50:31.0 -- not an asteroid (will add it to exclusion list)
20:06:22.34 +17:10:06.8 -- not an asteroid (will add it to exclusion list)
20:22:16.04 +21:24:01.9 -- not an asteroid (will add it to exclusion list)
20:02:16.65 +19:43:49.5 -- not an asteroid (will add it to exclusion list)
20:22:57.97 +22:38:12.4 -- not an asteroid (will add it to exclusion list)
19:49:57.29 +19:02:38.5 -- not an asteroid (will add it to exclusion list)
20:08:47.24 +18:26:44.2 -- not an asteroid (will add it to exclusion list)
19:53:38.83 +24:05:57.7 -- not an asteroid (will add it to exclusion list)
20:36:21.76 +24:58:36.7 -- not an asteroid (will add it to exclusion list)
20:13:05.15 +20:14:32.6 -- not an asteroid (will add it to exclusion list)
20:02:58.53 +23:53:35.8 -- not an asteroid (will add it to exclusion list)
20:11:51.46 +25:18:24.1 -- not an asteroid (will add it to exclusion list)
20:17:20.65 +23:50:18.4 -- not an asteroid (will add it to exclusion list)
20:47:44.13 +23:49:01.2 -- not an asteroid (will add it to exclusion list)
20:12:27.08 +20:16:49.3 -- not an asteroid (will add it to exclusion list)
19:51:16.41 +19:44:57.1 -- not an asteroid (will add it to exclusion list)
20:01:35.38 +18:44:45.7 -- not an asteroid (will add it to exclusion list)
19:57:52.87 +23:37:26.2 -- not an asteroid (will add it to exclusion list)
20:06:31.89 +19:27:39.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:46:30.71 +19:11:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:45.29 +18:57:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:09.52 +19:36:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:14.17 +21:05:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:18.37 +20:18:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:24.81 +23:50:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:34.74 +22:14:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:35.20 +21:24:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:50.55 +17:51:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:08.88 +18:51:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:12.58 +20:30:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:46.73 +18:44:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:54.38 +17:33:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:05.44 +21:17:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:42.38 +22:58:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:57.29 +19:02:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:14.56 +21:25:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:37.70 +21:28:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:37.72 +18:05:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:42.68 +17:24:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:42.88 +22:29:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:58.64 +17:38:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:09.11 +24:27:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:16.41 +19:44:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:20.03 +19:18:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:25.58 +21:29:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:28.71 +18:15:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:37.84 +18:13:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:41.19 +17:53:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:56.13 +20:31:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:56.44 +17:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:13.54 +18:20:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:21.45 +22:15:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:30.45 +17:51:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:37.20 +22:55:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:42.12 +20:41:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:56.70 +23:31:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:07.37 +22:01:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:38.83 +24:05:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:45.53 +19:16:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:48.78 +18:22:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:49.52 +20:17:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:51.32 +23:48:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:58.54 +17:48:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:04.90 +18:11:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:04.38 +22:55:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:05.05 +19:55:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:13.67 +22:56:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:16.79 +18:07:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:21.50 +20:26:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:53.02 +23:08:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:26.87 +19:38:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.15 +23:26:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:43.00 +20:09:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:47.99 +22:19:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:29.25 +19:17:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:35.40 +20:04:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:36.48 +21:11:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:42.24 +18:21:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:52.87 +23:37:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:54.00 +19:33:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:02.90 +22:49:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:06.44 +17:28:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:07.09 +22:16:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:26.46 +17:50:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:29.67 +20:53:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:35.62 +21:48:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:35.63 +19:10:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:42.65 +20:54:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:01.04 +24:41:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:05.59 +17:11:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:07.17 +19:34:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:36.58 +21:21:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:37.93 +22:44:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:47.11 +18:37:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:52.28 +24:38:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:00.39 +17:41:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.88 +22:46:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:21.53 +18:35:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:22.88 +17:40:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:35.84 +17:28:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.54 +18:34:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:41.51 +22:02:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:44.84 +21:05:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:54.89 +25:33:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:56.58 +21:55:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:00.99 +21:11:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:07.73 +19:25:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:09.13 +23:39:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:12.90 +19:29:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:25.53 +17:44:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:26.99 +21:15:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:29.96 +19:31:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:30.29 +24:27:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:35.38 +18:44:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:50.06 +22:49:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:58.45 +21:25:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:13.53 +20:09:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:14.15 +17:48:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:16.65 +19:43:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:21.20 +20:05:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:22.52 +18:23:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:28.78 +25:37:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:46.80 +22:04:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:57.04 +21:33:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:58.53 +23:53:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:01.51 +19:57:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:14.54 +20:58:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:24.79 +23:19:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:31.36 +19:13:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:45.07 +24:20:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:51.57 +18:04:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:06.93 +17:51:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:11.49 +19:17:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:12.73 +19:34:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:21.94 +17:48:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:26.41 +18:19:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:27.32 +22:37:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:28.49 +20:18:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:36.23 +21:28:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:44.14 +19:45:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:46.94 +21:35:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:09.47 +20:31:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:15.92 +17:40:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:38.82 +21:32:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:42.68 +21:20:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:47.38 +21:17:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:06.80 +21:49:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:22.34 +17:10:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:24.32 +17:59:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:31.89 +19:27:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:34.15 +20:21:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:35.06 +23:31:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:40.02 +25:01:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:40.13 +21:55:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:49.34 +18:43:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:12.87 +21:32:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:42.81 +23:54:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:52.72 +18:13:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:59.63 +21:53:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:02.30 +17:58:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:07.32 +17:37:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:07.41 +18:46:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:11.55 +19:18:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:15.77 +23:58:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:20.29 +23:35:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:26.50 +25:35:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:42.58 +17:43:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:47.24 +18:26:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:48.65 +24:30:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:49.05 +21:40:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:52.68 +24:28:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:56.44 +18:58:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:00.22 +20:18:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:34.60 +19:32:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:49.27 +17:24:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:50.96 +17:03:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:08.48 +23:34:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:37.48 +18:04:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:48.42 +17:08:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:53.63 +17:55:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:01.54 +17:14:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:37.52 +21:02:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:42.55 +21:51:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:42.66 +17:12:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:51.46 +25:18:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:01.84 +20:49:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:14.11 +19:04:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:24.55 +18:18:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:27.08 +20:16:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:33.13 +19:36:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:05.15 +20:14:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:20.37 +18:11:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:22.85 +21:03:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:31.14 +24:50:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:37.75 +18:40:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:47.80 +23:32:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:52.49 +20:09:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:05.43 +24:45:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:07.94 +17:40:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:09.78 +18:48:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:26.33 +17:05:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:33.38 +23:02:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:35.27 +26:27:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:36.70 +23:14:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:39.33 +18:26:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:51.36 +19:48:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:56.46 +24:39:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:59.13 +22:07:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:04.38 +23:54:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:15.94 +22:17:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:23.53 +21:45:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:25.09 +24:10:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:31.03 +20:39:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:37.93 +22:27:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:40.54 +21:31:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:40.71 +23:47:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:47.96 +21:47:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:49.24 +21:07:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:20.87 +18:55:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:41.67 +26:56:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:52.92 +21:20:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:59.05 +21:52:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:06.55 +22:45:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:20.65 +23:50:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:22.11 +21:22:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:25.16 +17:25:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:28.95 +22:57:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:50.60 +19:30:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:06.30 +20:17:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:02.63 +18:23:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:34.22 +17:59:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:49.88 +17:26:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:31.49 +18:58:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:42.72 +20:18:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:54.23 +18:21:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:57.86 +20:06:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:23.22 +22:01:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:24.87 +20:54:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:30.30 +24:32:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:43.46 +26:53:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:44.75 +20:47:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:49.11 +23:37:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:14.85 +23:48:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:16.04 +21:24:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:57.97 +22:38:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:34.94 +22:27:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:38.98 +17:53:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:40.99 +17:17:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:02.63 +24:58:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:15.28 +22:58:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:21.49 +17:58:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:30.66 +20:19:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:31.54 +17:33:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:38.37 +24:35:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:40.66 +22:39:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:00.19 +19:13:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:29.98 +20:44:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:31.86 +20:03:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:45.09 +19:55:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:53.94 +19:00:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:55.22 +25:47:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:58.51 +24:48:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:04.45 +20:46:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:19.91 +21:56:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:50.19 +24:43:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:00.20 +17:20:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:11.28 +23:14:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:19.96 +18:49:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:28.19 +24:17:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:59.17 +19:58:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:04.24 +26:55:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:30.55 +18:22:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:10.53 +22:28:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:15.90 +25:38:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:17.23 +26:17:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:26.73 +19:53:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:35.15 +23:15:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:19.32 +21:06:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:37.66 +18:47:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:41.06 +24:21:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:31:12.49 +26:12:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:31:40.28 +17:26:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:01.45 +18:20:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:04.56 +18:24:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:06.82 +20:39:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:24.59 +19:29:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:28.67 +19:48:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:16.98 +19:33:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:44.74 +26:03:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:48.60 +20:48:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:54.20 +20:27:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:00.58 +20:58:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:33.56 +20:18:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:42.16 +25:29:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:00.54 +20:30:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:21.76 +24:58:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:34.35 +18:05:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:01.79 +17:33:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:17.17 +25:02:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:21.60 +24:34:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:33.17 +20:03:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:47.50 +20:11:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:28.13 +22:13:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:43.97 +18:56:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:44.55 +18:56:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:41.30 +21:03:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:02.35 +23:49:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:16.93 +23:01:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:19.63 +25:45:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:37.45 +18:31:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:14.72 +25:13:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:30.33 +17:39:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:06.34 +23:22:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:50.00 +22:19:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:32.05 +20:43:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:41.25 +17:08:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:44.13 +23:49:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:59.39 +18:18:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:11.43 +20:19:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:43.15 +18:50:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:18.71 +20:05:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:21.64 +19:35:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:30.70 +23:34:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:47.34 +20:24:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:50.88 +19:51:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:19.98 +22:17:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:57.44 +23:54:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:31.78 +25:28:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:46:30.71 +19:11:21.9 -- a known variable star
19:46:45.29 +18:57:12.3 -- a known variable star
19:47:09.52 +19:36:09.5 -- a known variable star
19:47:14.17 +21:05:38.4 -- a known variable star
19:47:18.37 +20:18:06.6 -- a known variable star
19:47:24.81 +23:50:31.0 -- a known variable star
19:47:34.74 +22:14:35.1 -- not a known variable star
19:47:35.20 +21:24:58.4 -- a known variable star
19:47:50.55 +17:51:15.5 -- a known variable star
19:48:08.88 +18:51:21.4 -- a known variable star
19:48:12.58 +20:30:11.6 -- a known variable star
19:48:46.73 +18:44:48.9 -- a known variable star
19:48:54.38 +17:33:43.7 -- a known variable star
19:49:05.44 +21:17:34.0 -- a known variable star
19:49:42.38 +22:58:05.5 -- a known variable star
19:49:57.29 +19:02:38.5 -- a known variable star
19:50:14.56 +21:25:09.8 -- a known variable star
19:50:37.70 +21:28:40.0 -- not a known variable star
19:50:37.72 +18:05:40.8 -- a known variable star
19:50:42.68 +17:24:25.0 -- not a known variable star
19:50:42.88 +22:29:43.1 -- a known variable star
19:50:58.64 +17:38:58.1 -- a known variable star
19:51:09.11 +24:27:56.2 -- a known variable star
19:51:16.41 +19:44:57.1 -- not a known variable star
19:51:20.03 +19:18:23.3 -- not a known variable star
19:51:25.58 +21:29:31.4 -- a known variable star
19:51:28.71 +18:15:18.4 -- not a known variable star
19:51:37.84 +18:13:32.8 -- a known variable star
19:51:41.19 +17:53:36.6 -- not a known variable star
19:51:56.13 +20:31:52.2 -- a known variable star
19:51:56.44 +17:20:02.8 -- not a known variable star
19:52:13.54 +18:20:10.4 -- a known variable star
19:52:21.45 +22:15:52.9 -- a known variable star
19:52:30.45 +17:51:19.2 -- a known variable star
19:52:37.20 +22:55:47.6 -- a known variable star
19:52:42.12 +20:41:22.5 -- a known variable star
19:52:56.70 +23:31:31.8 -- a known variable star
19:53:07.37 +22:01:46.0 -- a known variable star
19:53:38.83 +24:05:57.7 -- a known variable star
19:53:45.53 +19:16:51.9 -- a known variable star
19:53:48.78 +18:22:01.7 -- a known variable star
19:53:49.52 +20:17:54.6 -- not a known variable star
19:53:51.32 +23:48:33.2 -- a known variable star
19:53:58.54 +17:48:12.2 -- a known variable star
19:54:04.90 +18:11:17.9 -- a known variable star
19:55:04.38 +22:55:52.9 -- a known variable star
19:55:05.05 +19:55:03.2 -- not a known variable star
19:55:13.67 +22:56:15.2 -- a known variable star
19:55:16.79 +18:07:45.3 -- a known variable star
19:55:21.50 +20:26:20.7 -- a known variable star
19:55:53.02 +23:08:11.0 -- a known variable star
19:56:26.87 +19:38:44.8 -- a known variable star
19:56:31.15 +23:26:10.2 -- a known variable star
19:56:43.00 +20:09:57.2 -- a known variable star
19:56:47.99 +22:19:39.1 -- a known variable star
19:57:29.25 +19:17:29.0 -- a known variable star
19:57:35.40 +20:04:54.8 -- a known variable star
19:57:36.48 +21:11:04.8 -- not a known variable star
19:57:42.24 +18:21:42.3 -- a known variable star
19:57:52.87 +23:37:26.2 -- a known variable star
19:57:54.00 +19:33:34.2 -- a known variable star
19:58:02.90 +22:49:27.2 -- a known variable star
19:58:06.44 +17:28:45.7 -- a known variable star
19:58:07.09 +22:16:03.0 -- a known variable star
19:58:26.46 +17:50:44.3 -- a known variable star
19:58:29.67 +20:53:09.5 -- not a known variable star
19:58:35.62 +21:48:06.5 -- a known variable star
19:58:35.63 +19:10:06.4 -- a known variable star
19:58:42.65 +20:54:21.1 -- a known variable star
19:59:01.04 +24:41:25.0 -- a known variable star
19:59:05.59 +17:11:03.3 -- a known variable star
19:59:07.17 +19:34:09.3 -- not a known variable star
19:59:36.58 +21:21:44.1 -- a known variable star
19:59:37.93 +22:44:01.4 -- a known variable star
19:59:47.11 +18:37:37.5 -- a known variable star
19:59:52.28 +24:38:51.2 -- a known variable star
20:00:00.39 +17:41:20.4 -- a known variable star
20:00:02.88 +22:46:48.2 -- a known variable star
20:00:21.53 +18:35:40.9 -- a known variable star
20:00:22.88 +17:40:17.3 -- not a known variable star
20:00:35.84 +17:28:08.3 -- a known variable star
20:00:37.54 +18:34:16.2 -- a known variable star
20:00:41.51 +22:02:42.2 -- a known variable star
20:00:44.84 +21:05:03.3 -- a known variable star
20:00:54.89 +25:33:41.5 -- not a known variable star
20:00:56.58 +21:55:32.7 -- a known variable star
20:01:00.99 +21:11:52.2 -- a known variable star
20:01:07.73 +19:25:34.4 -- a known variable star
20:01:09.13 +23:39:09.7 -- a known variable star
20:01:12.90 +19:29:37.7 -- a known variable star
20:01:25.53 +17:44:55.4 -- a known variable star
20:01:26.99 +21:15:51.6 -- a known variable star
20:01:29.96 +19:31:49.9 -- not a known variable star
20:01:30.29 +24:27:53.8 -- a known variable star
20:01:35.38 +18:44:45.7 -- a known variable star
20:01:50.06 +22:49:02.4 -- a known variable star
20:01:58.45 +21:25:01.4 -- a known variable star
20:02:13.53 +20:09:24.4 -- a known variable star
20:02:14.15 +17:48:58.6 -- a known variable star
20:02:16.65 +19:43:49.5 -- a known variable star
20:02:21.20 +20:05:14.6 -- a known variable star
20:02:22.52 +18:23:49.3 -- a known variable star
20:02:28.78 +25:37:35.8 -- not a known variable star
20:02:46.80 +22:04:59.4 -- a known variable star
20:02:57.04 +21:33:05.6 -- a known variable star
20:02:58.53 +23:53:35.8 -- a known variable star
20:03:01.51 +19:57:20.6 -- a known variable star
20:03:14.54 +20:58:56.9 -- a known variable star
20:03:24.79 +23:19:49.9 -- a known variable star
20:03:31.36 +19:13:13.5 -- a known variable star
20:03:45.07 +24:20:40.3 -- a known variable star
20:03:51.57 +18:04:50.6 -- a known variable star
20:04:06.93 +17:51:13.9 -- a known variable star
20:04:11.49 +19:17:58.7 -- not a known variable star
20:04:12.73 +19:34:24.4 -- a known variable star
20:04:21.94 +17:48:39.9 -- a known variable star
20:04:26.41 +18:19:43.0 -- a known variable star
20:04:27.32 +22:37:43.0 -- a known variable star
20:04:28.49 +20:18:28.5 -- not a known variable star
20:04:36.23 +21:28:14.2 -- a known variable star
20:04:44.14 +19:45:32.4 -- a known variable star
20:04:46.94 +21:35:49.5 -- a known variable star
20:05:09.47 +20:31:30.8 -- a known variable star
20:05:15.92 +17:40:53.4 -- a known variable star
20:05:38.82 +21:32:33.3 -- a known variable star
20:05:42.68 +21:20:25.8 -- a known variable star
20:05:47.38 +21:17:58.7 -- a known variable star
20:06:06.80 +21:49:46.5 -- a known variable star
20:06:22.34 +17:10:06.8 -- a known variable star
20:06:24.32 +17:59:01.0 -- a known variable star
20:06:31.89 +19:27:39.3 -- a known variable star
20:06:34.15 +20:21:40.7 -- a known variable star
20:06:35.06 +23:31:20.9 -- a known variable star
20:06:40.02 +25:01:29.2 -- a known variable star
20:06:40.13 +21:55:53.7 -- not a known variable star
20:06:49.34 +18:43:43.3 -- not a known variable star
20:07:12.87 +21:32:00.6 -- a known variable star
20:07:42.81 +23:54:51.9 -- a known variable star
20:07:52.72 +18:13:35.3 -- a known variable star
20:07:59.63 +21:53:59.1 -- a known variable star
20:08:02.30 +17:58:46.3 -- a known variable star
20:08:07.32 +17:37:17.6 -- a known variable star
20:08:07.41 +18:46:14.8 -- a known variable star
20:08:11.55 +19:18:21.3 -- a known variable star
20:08:15.77 +23:58:00.7 -- a known variable star
20:08:20.29 +23:35:11.7 -- a known variable star
20:08:26.50 +25:35:49.5 -- a known variable star
20:08:42.58 +17:43:52.8 -- a known variable star
20:08:47.24 +18:26:44.2 -- a known variable star
20:08:48.65 +24:30:26.5 -- a known variable star
20:08:49.05 +21:40:22.9 -- not a known variable star
20:08:52.68 +24:28:02.6 -- a known variable star
20:08:56.44 +18:58:02.8 -- not a known variable star
20:09:00.22 +20:18:27.6 -- a known variable star
20:09:34.60 +19:32:28.4 -- a known variable star
20:09:49.27 +17:24:16.9 -- a known variable star
20:09:50.96 +17:03:02.2 -- a known variable star
20:10:08.48 +23:34:32.2 -- a known variable star
20:10:37.48 +18:04:58.2 -- a known variable star
20:10:48.42 +17:08:59.0 -- a known variable star
20:10:53.63 +17:55:01.9 -- a known variable star
20:11:01.54 +17:14:38.0 -- a known variable star
20:11:37.52 +21:02:44.1 -- a known variable star
20:11:42.55 +21:51:05.0 -- a known variable star
20:11:42.66 +17:12:40.1 -- a known variable star
20:11:51.46 +25:18:24.1 -- not a known variable star
20:12:01.84 +20:49:41.6 -- a known variable star
20:12:14.11 +19:04:34.6 -- not a known variable star
20:12:24.55 +18:18:53.1 -- a known variable star
20:12:27.08 +20:16:49.3 -- a known variable star
20:12:33.13 +19:36:58.2 -- not a known variable star
20:13:05.15 +20:14:32.6 -- a known variable star
20:13:20.37 +18:11:32.2 -- a known variable star
20:13:22.85 +21:03:20.2 -- a known variable star
20:13:31.14 +24:50:33.4 -- a known variable star
20:13:37.75 +18:40:11.8 -- not a known variable star
20:13:47.80 +23:32:49.4 -- a known variable star
20:13:52.49 +20:09:59.7 -- a known variable star
20:14:05.43 +24:45:50.4 -- a known variable star
20:14:07.94 +17:40:56.6 -- a known variable star
20:14:09.78 +18:48:00.9 -- a known variable star
20:14:26.33 +17:05:17.5 -- a known variable star
20:14:33.38 +23:02:32.8 -- not a known variable star
20:14:35.27 +26:27:12.8 -- a known variable star
20:14:36.70 +23:14:36.6 -- a known variable star
20:14:39.33 +18:26:56.8 -- a known variable star
20:14:51.36 +19:48:06.1 -- not a known variable star
20:14:56.46 +24:39:28.8 -- a known variable star
20:14:59.13 +22:07:06.2 -- a known variable star
20:15:04.38 +23:54:56.2 -- a known variable star
20:15:15.94 +22:17:16.9 -- a known variable star
20:15:23.53 +21:45:01.1 -- a known variable star
20:15:25.09 +24:10:03.7 -- a known variable star
20:15:31.03 +20:39:23.5 -- a known variable star
20:15:37.93 +22:27:06.7 -- a known variable star
20:15:40.54 +21:31:15.9 -- a known variable star
20:15:40.71 +23:47:45.6 -- a known variable star
20:15:47.96 +21:47:52.0 -- a known variable star
20:15:49.24 +21:07:56.2 -- a known variable star
20:16:20.87 +18:55:29.1 -- a known variable star
20:16:41.67 +26:56:03.6 -- not a known variable star
20:16:52.92 +21:20:21.2 -- a known variable star
20:16:59.05 +21:52:31.0 -- a known variable star
20:17:06.55 +22:45:42.7 -- a known variable star
20:17:20.65 +23:50:18.4 -- a known variable star
20:17:22.11 +21:22:41.6 -- a known variable star
20:17:25.16 +17:25:58.8 -- a known variable star
20:17:28.95 +22:57:50.9 -- a known variable star
20:17:50.60 +19:30:03.0 -- a known variable star
20:18:06.30 +20:17:16.1 -- a known variable star
20:19:02.63 +18:23:10.6 -- not a known variable star
20:19:34.22 +17:59:12.0 -- a known variable star
20:19:49.88 +17:26:05.2 -- a known variable star
20:20:31.49 +18:58:09.9 -- a known variable star
20:20:42.72 +20:18:49.8 -- a known variable star
20:20:54.23 +18:21:22.8 -- a known variable star
20:20:57.86 +20:06:52.4 -- a known variable star
20:21:23.22 +22:01:46.3 -- a known variable star
20:21:24.87 +20:54:36.1 -- a known variable star
20:21:30.30 +24:32:50.4 -- a known variable star
20:21:43.46 +26:53:41.8 -- a known variable star
20:21:44.75 +20:47:34.1 -- a known variable star
20:21:49.11 +23:37:08.6 -- a known variable star
20:22:14.85 +23:48:13.0 -- a known variable star
20:22:16.04 +21:24:01.9 -- a known variable star
20:22:57.97 +22:38:12.4 -- a known variable star
20:23:34.94 +22:27:34.5 -- a known variable star
20:23:38.98 +17:53:35.3 -- a known variable star
20:23:40.99 +17:17:39.1 -- a known variable star
20:24:02.63 +24:58:50.2 -- a known variable star
20:24:15.28 +22:58:55.4 -- a known variable star
20:24:21.49 +17:58:51.3 -- a known variable star
20:24:30.66 +20:19:50.2 -- a known variable star
20:24:31.54 +17:33:52.7 -- not a known variable star
20:24:38.37 +24:35:27.4 -- a known variable star
20:24:40.66 +22:39:03.7 -- a known variable star
20:25:00.19 +19:13:05.7 -- a known variable star
20:25:29.98 +20:44:57.3 -- a known variable star
20:25:31.86 +20:03:07.8 -- a known variable star
20:25:45.09 +19:55:45.7 -- a known variable star
20:25:53.94 +19:00:51.0 -- not a known variable star
20:25:55.22 +25:47:16.2 -- not a known variable star
20:25:58.51 +24:48:41.8 -- a known variable star
20:26:04.45 +20:46:13.2 -- a known variable star
20:26:19.91 +21:56:40.5 -- a known variable star
20:26:50.19 +24:43:12.7 -- a known variable star
20:27:00.20 +17:20:14.8 -- a known variable star
20:27:11.28 +23:14:15.3 -- not a known variable star
20:27:19.96 +18:49:58.7 -- a known variable star
20:27:28.19 +24:17:20.6 -- a known variable star
20:27:59.17 +19:58:15.2 -- not a known variable star
20:28:04.24 +26:55:18.8 -- a known variable star
20:28:30.55 +18:22:09.4 -- not a known variable star
20:29:10.53 +22:28:13.9 -- not a known variable star
20:29:15.90 +25:38:39.7 -- a known variable star
20:29:17.23 +26:17:26.5 -- a known variable star
20:29:26.73 +19:53:18.7 -- a known variable star
20:29:35.15 +23:15:55.1 -- a known variable star
20:30:19.32 +21:06:49.1 -- a known variable star
20:30:37.66 +18:47:46.1 -- a known variable star
20:30:41.06 +24:21:46.7 -- a known variable star
20:31:12.49 +26:12:24.7 -- a known variable star
20:31:40.28 +17:26:06.1 -- a known variable star
20:32:01.45 +18:20:33.1 -- a known variable star
20:32:04.56 +18:24:25.3 -- a known variable star
20:32:06.82 +20:39:07.1 -- a known variable star
20:32:24.59 +19:29:38.6 -- a known variable star
20:32:28.67 +19:48:51.0 -- a known variable star
20:33:16.98 +19:33:27.4 -- not a known variable star
20:33:44.74 +26:03:25.1 -- a known variable star
20:33:48.60 +20:48:07.2 -- a known variable star
20:33:54.20 +20:27:24.2 -- a known variable star
20:34:00.58 +20:58:41.9 -- a known variable star
20:34:33.56 +20:18:15.2 -- a known variable star
20:35:42.16 +25:29:11.7 -- a known variable star
20:36:00.54 +20:30:03.7 -- a known variable star
20:36:21.76 +24:58:36.7 -- a known variable star
20:36:34.35 +18:05:21.6 -- a known variable star
20:37:01.79 +17:33:04.4 -- a known variable star
20:37:17.17 +25:02:14.3 -- a known variable star
20:37:21.60 +24:34:07.0 -- not a known variable star
20:37:33.17 +20:03:17.4 -- a known variable star
20:38:47.50 +20:11:01.1 -- not a known variable star
20:40:28.13 +22:13:09.4 -- a known variable star
20:40:43.97 +18:56:32.8 -- a known variable star
20:40:44.55 +18:56:26.6 -- a known variable star
20:41:41.30 +21:03:29.5 -- not a known variable star
20:43:02.35 +23:49:30.0 -- a known variable star
20:43:16.93 +23:01:32.0 -- a known variable star
20:43:19.63 +25:45:32.0 -- a known variable star
20:43:37.45 +18:31:30.0 -- a known variable star
20:44:14.72 +25:13:23.8 -- a known variable star
20:44:30.33 +17:39:27.6 -- not a known variable star
20:45:06.34 +23:22:32.1 -- a known variable star
20:45:50.00 +22:19:09.2 -- not a known variable star
20:47:32.05 +20:43:38.9 -- not a known variable star
20:47:41.25 +17:08:04.0 -- not a known variable star
20:47:44.13 +23:49:01.2 -- not a known variable star
20:47:59.39 +18:18:46.3 -- a known variable star
20:48:11.43 +20:19:40.8 -- not a known variable star
20:48:43.15 +18:50:39.7 -- not a known variable star
20:49:18.71 +20:05:13.0 -- not a known variable star
20:49:21.64 +19:35:34.8 -- not a known variable star
20:49:30.70 +23:34:56.9 -- a known variable star
20:49:47.34 +20:24:36.3 -- a known variable star
20:49:50.88 +19:51:11.4 -- not a known variable star
20:50:19.98 +22:17:41.9 -- a known variable star
20:50:57.44 +23:54:03.5 -- a known variable star
20:52:31.78 +25:28:10.0 -- not a known variable star
Found 53 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
309 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 309 (excluding asteroids and hot pixels, 53 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461139.86544341 -observatory V36
23:34:24.93 -05:15:22.9 Mercury (0.2mag)
02:36:34.69 +15:12:53.0 Venus (-3.9mag)
23:58:58.04 -01:12:51.5 Mars (1.2mag)
07:09:51.25 +22:50:40.0 Jupiter (-2.1mag)
00:26:12.10 +00:30:18.5 Saturn (0.9mag)
03:46:20.41 +19:43:06.0 Uranus (5.8mag)
00:09:57.57 -00:20:56.5 Neptune (7.8mag)
20:33:25.43 -22:52:26.9 Pluto (14.5mag)
18:47:28.77 -28:03:17.5 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Apr 9 03:53 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461139.86544341:
07:09:59.04 +22:50:25.0 Io (5.7mag)
07:10:02.47 +22:50:18.2 Europa (5.9mag)
07:10:03.48 +22:50:09.3 Ganymede (5.3mag)
07:09:22.15 +22:51:42.5 Callisto (6.5mag)
07:13:27.64 +22:41:31.4 Himalia (15.3mag)
07:09:49.45 +22:50:41.4 Thebe (16.2mag)
07:13:29.95 +23:10:55.1 Elara (17.3mag)
07:08:17.05 +23:34:08.6 Pasiphae (17.4mag)
07:18:19.39 +22:47:59.0 Carme (18.5mag)
00:26:19.49 +00:30:07.8 Titan (8.8mag)
00:26:15.89 +00:30:29.5 Rhea (10.1mag)
00:26:05.44 +00:31:28.2 Iapetus (11.5mag)
00:26:23.95 +00:30:05.2 Hyperion (14.8mag)
00:27:54.06 +00:39:48.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 03:53 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.86544341:
15:04:48.20 -11:09:33.3 JWST
17:52:22.98 +37:09:41.1 Chandra
18:55:19.80 -16:08:10.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 03:53 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.86544341 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:54.11 -28:24:16.2 13.9mag P/2010 H2 (Vales)
05:02:08.60 -69:59:08.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:07.14 +31:23:40.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.19 +09:45:15.6 17.6mag C/2021 G2 (ATLAS)
23:08:20.54 +28:58:40.4 17.0mag C/2022 E2 (ATLAS)
04:21:35.15 +25:51:16.5 15.9mag C/2022 N2 (PANSTARRS)
09:02:14.28 +31:57:18.5 16.2mag C/2022 QE78 (ATLAS)
08:30:14.30 -00:52:26.1 17.3mag C/2022 R6 (PANSTARRS)
18:55:05.87 +17:58:07.8 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:40.52 -11:37:01.4 17.6mag P/2023 B1 (PANSTARRS)
09:10:59.79 -12:58:04.9 17.6mag C/2023 F3 (ATLAS)
21:47:09.63 +62:32:06.2 17.5mag C/2023 H5 (Lemmon)
19:24:21.89 -03:38:26.4 14.2mag C/2023 R1 (PANSTARRS)
21:41:11.33 +85:00:57.8 17.8mag C/2023 X2 (Lemmon)
06:15:19.76 +63:33:15.8 17.1mag C/2024 A1 (ATLAS)
04:58:32.88 +15:53:29.5 10.6mag C/2024 E1 (Wierzchos)
16:23:19.96 +05:18:00.1 17.4mag C/2024 G6 (ATLAS)
20:18:43.39 +13:30:16.2 14.7mag C/2024 J3 (ATLAS)
03:20:30.01 -23:24:54.0 16.4mag C/2024 T5 (ATLAS)
05:11:13.00 +46:59:05.4 17.7mag C/2025 J1 (Borisov)
14:06:18.80 +40:24:31.7 14.9mag C/2025 L1 (ATLAS)
03:15:03.23 -25:12:24.7 17.8mag C/2025 Q3 (ATLAS)
23:03:31.81 +19:45:45.4 9.6mag C/2025 R3 (PANSTARRS)
12:57:00.41 +02:35:53.6 17.5mag C/2025 Y1 (ATLAS)
02:19:49.27 +03:41:11.0 10.4mag C/2026 A1 (MAPS)
23:40:20.77 +35:55:29.7 14.4mag C/2026 B2 (Sun-Gao)
18:29:59.77 -10:03:52.1 12.2mag 10P/Tempel
15:09:01.68 +03:50:50.9 13.4mag 24P/Schaumasse
11:04:43.81 -01:44:59.6 15.7mag 29P/Schwassmann-Wachmann
17:58:26.46 -09:51:53.9 17.8mag 40P/Vaisala
10:38:14.25 -04:39:27.3 16.8mag 43P/Wolf-Harrington
01:38:25.86 +16:20:53.1 17.2mag 47P/Ashbrook-Jackson
06:58:48.16 +38:25:12.6 17.0mag 63P/Wild
23:20:29.52 -12:15:34.0 15.7mag 65P/Gunn
03:45:48.07 +18:54:35.3 15.9mag 76P/West-Kohoutek-Ikemura
00:50:59.43 +06:55:02.6 14.4mag 78P/Gehrels
22:42:35.18 -11:20:47.7 14.6mag 88P/Howell
01:51:51.38 +18:50:14.8 15.1mag 93P/Lovas
04:42:33.70 +31:55:02.1 16.3mag 123P/West-Hartley
08:21:01.24 +41:25:27.2 16.2mag 124P/Mrkos
02:23:01.90 +13:37:17.2 16.4mag 128P/Shoemaker-Holt
02:34:33.99 +13:39:53.4 17.5mag 131P/Mueller
00:51:50.12 +10:50:02.7 11.0mag 141P/Machholz
01:01:33.21 +02:22:54.9 11.0mag 141P-A/Machholz
23:50:17.70 -01:24:59.2 13.6mag 141P-D/Machholz
01:31:09.32 +04:05:35.1 17.9mag 141P-I/Machholz
00:43:55.79 -04:50:49.1 15.2mag 162P/SidingSpring
10:30:02.91 +31:18:25.0 17.9mag 164P/Christensen
06:24:15.02 +24:26:37.3 17.9mag 198P/ODAS
15:03:11.19 -00:48:20.0 17.4mag 210P/Christensen
21:18:58.45 -13:03:16.0 17.5mag 218P/LINEAR
17:14:14.32 -14:42:54.6 16.2mag 235P/LINEAR
05:20:18.35 +34:09:08.0 16.6mag 240P/NEAT
07:35:27.60 -05:54:39.6 17.7mag 242P/Spahr
15:45:00.11 +06:32:13.4 17.5mag 391P/Kowalski
07:31:51.55 +21:20:05.6 17.6mag 450P/LONEOS
05:26:20.56 +45:25:20.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 03:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 9 03:53 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 9 03:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:50:43.720 +47:30:42.19 AT 2026ify 2026-03-30.81 21.34
17:38:02.570 +25:54:11.91 AT 2026ifx 2026-03-27.88 20.89
16:42:02.490 +40:59:30.50 AT 2026ifw 2026-03-27.86 21.32
16:24:14.050 +39:37:35.59 AT 2026ifv 2026-03-27.86 20.81
16:16:45.660 +38:01:36.33 AT 2026ifu 2026-03-27.86 21.15
16:28:23.190 +36:11:26.67 AT 2026ift 2026-03-27.86 21.53
16:16:10.610 +36:40:26.87 AT 2026ifs 2026-03-27.86 20.03
16:42:08.700 +33:28:34.26 AT 2026ifr 2026-03-27.86 21.24
16:45:41.760 +34:10:06.31 AT 2026ifq 2026-03-27.86 21.64
16:50:17.550 +33:04:52.33 AT 2026ifp 2026-03-27.86 19.99
16:52:21.140 +31:25:32.03 AT 2026ifo 2026-03-27.86 19.73
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
16:26:20.250 +28:06:35.30 AT 2026ifm 2026-03-27.85 20.13
17:01:36.800 +29:43:13.81 AT 2026ifl 2026-03-27.85 20.62
17:06:26.770 +28:47:25.16 AT 2026ifk 2026-03-27.85 21.39
16:47:18.680 +27:13:25.92 AT 2026ifj 2026-03-27.85 20.26
15:55:49.720 +37:36:32.33 AT 2026ifi 2026-03-24.80 21.32
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
-rw-r--r-- 1 apache apache 30K Apr 9 03:53 tns_transients_list.txt
