This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978690000420371456,2461150.9279,10.20,0.05,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
Gaia DR3 5978690000420371456 20260420.4279 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980774124824395264,2461150.9279,10.11,0.05,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 5980774124824395264 20260420.4279 10.11CV 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
Gaia DR3 5973560984837725824,2461150.9279,9.92,0.05,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
Gaia DR3 5973560984837725824 20260420.4279 9.92CV 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
Gaia DR3 5976331578031237376,2461150.9279,9.85,0.05,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
Gaia DR3 5976331578031237376 20260420.4279 9.85CV 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
ASAS J171626-3117.0,2461150.9279,9.47,0.05,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
ASAS J171626-3117.0 20260420.4279 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030422602314419840,2461150.9279,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030422602314419840 20260420.4279 9.44CV 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
Gaia DR3 6030550592338002560,2461150.9279,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030550592338002560 20260420.4279 9.44CV 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
Gaia DR3 6020707047012971392,2461150.9279,9.55,0.05,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
Gaia DR3 6020707047012971392 20260420.4279 9.55CV 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
Gaia DR3 5972731918726009472,2461150.9279,9.69,0.05,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
Gaia DR3 5972731918726009472 20260420.4279 9.69CV 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
OGLE-BLG-LPV-233275,2461150.9279,9.74,0.05,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
OGLE-BLG-LPV-233275 20260420.4279 9.74CV 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
Gaia DR3 6028580203186347136,2461150.9279,9.82,0.05,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
Gaia DR3 6028580203186347136 20260420.4279 9.82CV 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
Gaia DR3 4059237912889903232,2461150.9279,9.82,0.05,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
Gaia DR3 4059237912889903232 20260420.4279 9.82CV 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
Gaia DR3 5972850769048992000,2461150.9279,9.88,0.05,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
Gaia DR3 5972850769048992000 20260420.4279 9.88CV 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
Gaia DR3 4107374295799436032,2461150.9279,9.98,0.05,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
Gaia DR3 4107374295799436032 20260420.4279 9.98CV 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
Gaia DR3 5972660411778306304,2461150.9279,9.99,0.05,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
Gaia DR3 5972660411778306304 20260420.4279 9.99CV 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 4059263132927790208,2461150.9279,10.08,0.05,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
Gaia DR3 4059263132927790208 20260420.4279 10.08CV 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
Gaia DR3 4059383877478772864,2461150.9279,10.09,0.05,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
Gaia DR3 4059383877478772864 20260420.4279 10.09CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 9.73 16:54:33.21 -38:05:47.5
346.41087 3.47331 galactic Sco Second-epoch detections are separated by 2.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5971248260889725824 | 16:54:34.07 -38:06:20.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A9V 1982MSS...C03....0H HD 152369 J-Ks=1.365+/-0.168 (Very red! L if it's a dwarf)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5971248260889725824,2461150.9279,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5971248260889725824 20260420.4279 9.73CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 9.89 17:17:58.57 -35:50:15.3
351.03402 1.09827 galactic Sco Second-epoch detections are separated by 3.6" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5975462487104036992 | 17:17:59.96 -35:50:29.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5975462487104036992,2461150.9279,9.89,0.05,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
Large-amplitude variable Gaia DR2 5975462487104036992 20260420.4279 9.89CV 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
Gaia DR3 4107315197030881664,2461150.9279,9.21,0.05,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 4107315197030881664 20260420.4279 9.21CV 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
Gaia DR3 6027989142556902016,2461150.9279,11.94,0.05,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
Gaia DR3 6027989142556902016 20260420.4279 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
Gaia DR3 6027252371017218432,2461150.9279,11.94,0.05,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
Gaia DR3 6027252371017218432 20260420.4279 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
Gaia DR3 6020086544495126016,2461150.9279,12.01,0.05,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
Gaia DR3 6020086544495126016 20260420.4279 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165948.70-294744.0,2461150.9279,11.75,0.05,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
ASASSN-V J165948.70-294744.0 20260420.4279 11.75CV 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
Gaia DR3 6024476447741446912,2461150.9279,11.76,0.05,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
Gaia DR3 6024476447741446912 20260420.4279 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037240506419058688,2461150.9279,11.64,0.05,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
Gaia DR3 6037240506419058688 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5978009059207638400,2461150.9279,11.86,0.05,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
Gaia DR3 5978009059207638400 20260420.4279 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
Gaia DR3 6021262536582158208,2461150.9279,11.79,0.05,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
Gaia DR3 6021262536582158208 20260420.4279 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6036703360623559552,2461150.9279,11.60,0.05,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 6036703360623559552 20260420.4279 11.60CV 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
Gaia DR3 6028374869378664064,2461150.9279,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6028374869378664064 20260420.4279 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
Gaia DR3 6036940889506286336,2461150.9279,11.47,0.05,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
Gaia DR3 6036940889506286336 20260420.4279 11.47CV 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
Gaia DR3 6038015352879148288,2461150.9279,11.40,0.05,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
Gaia DR3 6038015352879148288 20260420.4279 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 6019743737395319424,2461150.9279,11.70,0.05,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
Gaia DR3 6019743737395319424 20260420.4279 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
VARIABLE_NAME,2461150.9279,11.43,0.05,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
VARIABLE_NAME 20260420.4279 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
Gaia DR3 6024319556860615808,2461150.9279,11.30,0.05,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
Gaia DR3 6024319556860615808 20260420.4279 11.30CV 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 5971261150144105984,2461150.9279,11.76,0.05,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
Gaia DR3 5971261150144105984 20260420.4279 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J162035.20-321739.9,2461150.9279,11.26,0.05,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
ASASSN-V J162035.20-321739.9 20260420.4279 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
Gaia DR3 5973523154763482240,2461150.9279,12.01,0.05,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
Gaia DR3 5973523154763482240 20260420.4279 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6035937104110268544,2461150.9279,11.38,0.05,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 6035937104110268544 20260420.4279 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6021265667640459520,2461150.9279,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6021265667640459520 20260420.4279 11.32CV 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
Gaia DR3 6024155145514185600,2461150.9279,11.37,0.05,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
Gaia DR3 6024155145514185600 20260420.4279 11.37CV 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
Gaia DR3 6027216598203106688,2461150.9279,11.45,0.05,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
Gaia DR3 6027216598203106688 20260420.4279 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
Gaia DR3 5977834099375225856,2461150.9279,11.41,0.05,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
Gaia DR3 5977834099375225856 20260420.4279 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
Gaia DR3 5971683156443464448,2461150.9279,11.43,0.05,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
Gaia DR3 5971683156443464448 20260420.4279 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
Gaia DR3 6023770733078935040,2461150.9279,11.21,0.05,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 6023770733078935040 20260420.4279 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
Gaia DR3 6038517211218299520,2461150.9279,11.03,0.05,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
Gaia DR3 6038517211218299520 20260420.4279 11.03CV 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
Gaia DR3 6038496694150609536,2461150.9279,11.26,0.05,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
Gaia DR3 6038496694150609536 20260420.4279 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
Gaia DR3 6024233627478683136,2461150.9279,11.34,0.05,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
Gaia DR3 6024233627478683136 20260420.4279 11.34CV 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 6037148181806392576,2461150.9279,11.24,0.05,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
Gaia DR3 6037148181806392576 20260420.4279 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038487696202814080,2461150.9279,11.00,0.05,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
Gaia DR3 6038487696202814080 20260420.4279 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6019388492055323520,2461150.9279,11.31,0.05,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
Gaia DR3 6019388492055323520 20260420.4279 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
VARIABLE_NAME,2461150.9279,11.13,0.05,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
VARIABLE_NAME 20260420.4279 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
VARIABLE_NAME,2461150.9279,11.11,0.05,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
VARIABLE_NAME 20260420.4279 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973151004436489600,2461150.9279,11.43,0.05,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
Gaia DR3 5973151004436489600 20260420.4279 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
Gaia DR3 6037002255999955840,2461150.9279,11.11,0.05,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
Gaia DR3 6037002255999955840 20260420.4279 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027416095175654912,2461150.9279,11.13,0.05,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
Gaia DR3 6027416095175654912 20260420.4279 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
Gaia DR3 5979469348040387200,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5979469348040387200 20260420.4279 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.6203-31.3907,2461150.9279,10.83,0.05,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
ATO J241.6203-31.3907 20260420.4279 10.83CV 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
Gaia DR3 5978638009824699136,2461150.9279,11.35,0.05,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
Gaia DR3 5978638009824699136 20260420.4279 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5970368926466312064,2461150.9279,11.31,0.05,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
Gaia DR3 5970368926466312064 20260420.4279 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 6038695538260027904,2461150.9279,11.05,0.05,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 6038695538260027904 20260420.4279 11.05CV 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 6024458168360450048,2461150.9279,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6024458168360450048 20260420.4279 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-LPV-000184,2461150.9279,11.07,0.05,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
OGLE-BLG-LPV-000184 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041695521382166656,2461150.9279,10.79,0.05,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
Gaia DR3 6041695521382166656 20260420.4279 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
Gaia DR3 6029439059201372288,2461150.9279,10.95,0.05,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 6029439059201372288 20260420.4279 10.95CV 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
Gaia DR3 5977952464320600192,2461150.9279,11.22,0.05,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
Gaia DR3 5977952464320600192 20260420.4279 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
Gaia DR3 5978650899056615680,2461150.9279,11.43,0.05,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
Gaia DR3 5978650899056615680 20260420.4279 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
Gaia DR3 5973561427198253184,2461150.9279,11.49,0.05,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 5973561427198253184 20260420.4279 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6036845231992515072,2461150.9279,10.82,0.05,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
Gaia DR3 6036845231992515072 20260420.4279 10.82CV 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
Gaia DR3 5973916882993172224,2461150.9279,11.23,0.05,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 5973916882993172224 20260420.4279 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 6028751692625416576,2461150.9279,10.97,0.05,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
Gaia DR3 6028751692625416576 20260420.4279 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
Gaia DR3 6027768385616591488,2461150.9279,10.89,0.05,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 6027768385616591488 20260420.4279 10.89CV 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
Gaia DR3 6024526574282353280,2461150.9279,11.03,0.05,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
Gaia DR3 6024526574282353280 20260420.4279 11.03CV 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
Gaia DR3 5979675162833159040,2461150.9279,11.13,0.05,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
Gaia DR3 5979675162833159040 20260420.4279 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 J165001.52-322539.9,2461150.9279,11.01,0.05,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 J165001.52-322539.9 20260420.4279 11.01CV 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
Gaia DR3 5978556134860212096,2461150.9279,11.06,0.05,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
Gaia DR3 5978556134860212096 20260420.4279 11.06CV 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
OGLE-BLG-LPV-235531,2461150.9279,11.11,0.05,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
OGLE-BLG-LPV-235531 20260420.4279 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041631715346885632,2461150.9279,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6041631715346885632 20260420.4279 10.81CV 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
Gaia DR3 5972744253873313792,2461150.9279,11.40,0.05,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
Gaia DR3 5972744253873313792 20260420.4279 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 5978561250173212288,2461150.9279,11.21,0.05,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 5978561250173212288 20260420.4279 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
Gaia DR3 5973979619578784512,2461150.9279,11.30,0.05,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
Gaia DR3 5973979619578784512 20260420.4279 11.30CV 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 5979733677584540032,2461150.9279,10.95,0.05,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 5979733677584540032 20260420.4279 10.95CV 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
Gaia DR3 5972710576999615104,2461150.9279,11.30,0.05,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
Gaia DR3 5972710576999615104 20260420.4279 11.30CV 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 J162406.63-330930.3,2461150.9279,10.83,0.05,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 J162406.63-330930.3 20260420.4279 10.83CV 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
Gaia DR3 5973480514339996544,2461150.9279,11.18,0.05,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
Gaia DR3 5973480514339996544 20260420.4279 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
Gaia DR3 5973104687505369088,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5973104687505369088 20260420.4279 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973533290888057984,2461150.9279,11.20,0.05,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
Gaia DR3 5973533290888057984 20260420.4279 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978204149409181824,2461150.9279,11.05,0.05,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 5978204149409181824 20260420.4279 11.05CV 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 J170953-3123.1,2461150.9279,10.97,0.05,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
ASAS J170953-3123.1 20260420.4279 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
Gaia DR3 5976526642580103680,2461150.9279,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5976526642580103680 20260420.4279 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J170216-2935.4,2461150.9279,10.77,0.05,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
ASAS J170216-2935.4 20260420.4279 10.77CV 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
Gaia DR3 5972674194364331008,2461150.9279,11.03,0.05,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
Gaia DR3 5972674194364331008 20260420.4279 11.03CV 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
Gaia DR3 5970584533833790976,2461150.9279,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5970584533833790976 20260420.4279 11.19CV 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
ASAS J170420-3451.0,2461150.9279,11.07,0.05,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
ASAS J170420-3451.0 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973845895784839168,2461150.9279,11.07,0.05,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 5973845895784839168 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973694060090451968,2461150.9279,11.08,0.05,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
Gaia DR3 5973694060090451968 20260420.4279 11.08CV 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
Gaia DR3 5972860114897897984,2461150.9279,11.21,0.05,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 5972860114897897984 20260420.4279 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
Gaia DR3 5978789643667159808,2461150.9279,11.04,0.05,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
Gaia DR3 5978789643667159808 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5972636841004448128,2461150.9279,11.16,0.05,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
Gaia DR3 5972636841004448128 20260420.4279 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5975556289190726912,2461150.9279,11.12,0.05,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 5975556289190726912 20260420.4279 11.12CV 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
GDS_J1707109-372937,2461150.9279,11.09,0.05,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
GDS_J1707109-372937 20260420.4279 11.09CV 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
Gaia DR3 5979074898249372288,2461150.9279,10.84,0.05,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 5979074898249372288 20260420.4279 10.84CV 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 5973247246058478848,2461150.9279,10.96,0.05,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 5973247246058478848 20260420.4279 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
Gaia DR3 5972733116984681344,2461150.9279,10.89,0.05,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 5972733116984681344 20260420.4279 10.89CV 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
Gaia DR3 5973634239788959616,2461150.9279,11.18,0.05,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
Gaia DR3 5973634239788959616 20260420.4279 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
Gaia DR3 5972735934482656512,2461150.9279,10.96,0.05,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 5972735934482656512 20260420.4279 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
ASAS J171010-3445.1,2461150.9279,10.68,0.05,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
ASAS J171010-3445.1 20260420.4279 10.68CV 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
Gaia DR3 5979511851017250688,2461150.9279,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5979511851017250688 20260420.4279 10.72CV 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
[HHR2012] J171920.1-371907,2461150.9279,10.88,0.05,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
[HHR2012] J171920.1-371907 20260420.4279 10.88CV 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
Gaia DR3 5973499343464922496,2461150.9279,10.76,0.05,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
Gaia DR3 5973499343464922496 20260420.4279 10.76CV 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 DR3 5967231092078478464,2461150.9279,10.71,0.05,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 5967231092078478464 20260420.4279 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
OGLE-BLG-LPV-235576,2461150.9279,10.67,0.05,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
OGLE-BLG-LPV-235576 20260420.4279 10.67CV 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
Gaia DR3 5976867383784091648,2461150.9279,10.42,0.05,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
Gaia DR3 5976867383784091648 20260420.4279 10.42CV 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
Gaia DR3 5972752839474492800,2461150.9279,10.66,0.05,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
Gaia DR3 5972752839474492800 20260420.4279 10.66CV 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 5973107298845565952,2461150.9279,10.60,0.05,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 5973107298845565952 20260420.4279 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973633346433006848,2461150.9279,10.53,0.05,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
Gaia DR3 5973633346433006848 20260420.4279 10.53CV 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
Gaia DR3 6027245121111467776,2461150.9279,9.43,0.05,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
Gaia DR3 6027245121111467776 20260420.4279 9.43CV 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
VARIABLE_NAME,2461150.9279,9.40,0.05,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
VARIABLE_NAME 20260420.4279 9.40CV 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 5978690000420371456,2461150.9279,10.01,0.05,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
Gaia DR3 5978690000420371456 20260420.4279 10.01CV 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
ASAS J171018-3719.5,2461150.9279,10.22,0.05,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
ASAS J171018-3719.5 20260420.4279 10.22CV 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 4107374566303607808,2461150.9279,9.89,0.05,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 4107374566303607808 20260420.4279 9.89CV 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
Gaia DR3 6028677303783760128,2461150.9279,10.03,0.05,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
Gaia DR3 6028677303783760128 20260420.4279 10.03CV 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
Gaia DR3 5980541371943816576,2461150.9279,10.07,0.05,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 5980541371943816576 20260420.4279 10.07CV 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
Gaia DR3 5976901060657658880,2461150.9279,10.35,0.05,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
Gaia DR3 5976901060657658880 20260420.4279 10.35CV 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
Gaia DR3 5976457442048675840,2461150.9279,10.38,0.05,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 5976457442048675840 20260420.4279 10.38CV 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
Gaia DR3 5978759819411997824,2461150.9279,10.34,0.05,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
Gaia DR3 5978759819411997824 20260420.4279 10.34CV 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 5980436368499346432,2461150.9279,10.20,0.05,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
Gaia DR3 5980436368499346432 20260420.4279 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J171207-2919.1,2461150.9279,10.12,0.05,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
ASAS J171207-2919.1 20260420.4279 10.12CV 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 5972781632935401728,2461150.9279,10.49,0.05,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 5972781632935401728 20260420.4279 10.49CV 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
Gaia DR3 4059181773466304256,2461150.9279,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4059181773466304256 20260420.4279 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029286428838464000,2461150.9279,10.16,0.05,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
Gaia DR3 6029286428838464000 20260420.4279 10.16CV 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
OGLE-BLG-ECL-004273,2461150.9279,10.32,0.05,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
OGLE-BLG-ECL-004273 20260420.4279 10.32CV 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
Gaia DR3 5978039089630066176,2461150.9279,10.47,0.05,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
Gaia DR3 5978039089630066176 20260420.4279 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980436368499346432,2461150.9279,10.36,0.05,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
Gaia DR3 5980436368499346432 20260420.4279 10.36CV 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
Gaia DR3 6028418162659991808,2461150.9279,10.40,0.05,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
Gaia DR3 6028418162659991808 20260420.4279 10.40CV 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 6041818735397001088,2461150.9279,10.27,0.05,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
Gaia DR3 6041818735397001088 20260420.4279 10.27CV 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 6026083693280040320,2461150.9279,10.46,0.05,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 6026083693280040320 20260420.4279 10.46CV 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 5979183264514743936,2461150.9279,10.59,0.05,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
Gaia DR3 5979183264514743936 20260420.4279 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
Gaia DR3 6028879987496149504,2461150.9279,10.30,0.05,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
Gaia DR3 6028879987496149504 20260420.4279 10.30CV 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 6029159435245468672,2461150.9279,10.30,0.05,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
Gaia DR3 6029159435245468672 20260420.4279 10.30CV 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 6041844848798515200,2461150.9279,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6041844848798515200 20260420.4279 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978415156962355712,2461150.9279,10.46,0.05,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 5978415156962355712 20260420.4279 10.46CV 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 5976605085896384896,2461150.9279,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5976605085896384896 20260420.4279 10.72CV 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
Gaia DR3 6026823836406402176,2461150.9279,10.52,0.05,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
Gaia DR3 6026823836406402176 20260420.4279 10.52CV 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 5978751813592647808,2461150.9279,10.59,0.05,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
Gaia DR3 5978751813592647808 20260420.4279 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
Gaia DR3 6042151887417564160,2461150.9279,10.21,0.05,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 6042151887417564160 20260420.4279 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029788016616087296,2461150.9279,10.45,0.05,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 6029788016616087296 20260420.4279 10.45CV 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
VARIABLE_NAME,2461150.9279,10.39,0.05,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
VARIABLE_NAME 20260420.4279 10.39CV 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 5979589327896715520,2461150.9279,10.58,0.05,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
Gaia DR3 5979589327896715520 20260420.4279 10.58CV 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
Gaia DR3 5978339153158426752,2461150.9279,10.70,0.05,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
Gaia DR3 5978339153158426752 20260420.4279 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973897297942246656,2461150.9279,10.88,0.05,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
Gaia DR3 5973897297942246656 20260420.4279 10.88CV 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
Gaia DR3 5973820744455929216,2461150.9279,10.87,0.05,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 5973820744455929216 20260420.4279 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5976329898734201472,2461150.9279,10.93,0.05,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 5976329898734201472 20260420.4279 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6027760753376135040,2461150.9279,10.62,0.05,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 6027760753376135040 20260420.4279 10.62CV 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
Gaia DR3 6030690264668982400,2461150.9279,10.53,0.05,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
Gaia DR3 6030690264668982400 20260420.4279 10.53CV 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
Gaia DR3 6029598965018664320,2461150.9279,10.55,0.05,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
Gaia DR3 6029598965018664320 20260420.4279 10.55CV 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
Gaia DR3 5971699786558352384,2461150.9279,10.85,0.05,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
Gaia DR3 5971699786558352384 20260420.4279 10.85CV 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
ATO J253.0200-29.7610,2461150.9279,10.65,0.05,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
ATO J253.0200-29.7610 20260420.4279 10.65CV 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
V1576 Sco,2461150.9279,10.63,0.05,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
V1576 Sco 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6024099040369661184,2461150.9279,10.61,0.05,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
Gaia DR3 6024099040369661184 20260420.4279 10.61CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 10.71 16:58:21.71 -32:42:10.4
351.13487 6.21922 galactic Sco Second-epoch detections are separated by 3.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6026802464644499840 | 16:58:21.60 -32:41:26.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6026802464644499840,2461150.9279,10.71,0.05,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
Large-amplitude variable Gaia DR2 6026802464644499840 20260420.4279 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
Gaia DR3 5980514330869711104,2461150.9279,10.76,0.05,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
Gaia DR3 5980514330869711104 20260420.4279 10.76CV 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
EPIC 202544292,2461150.9279,10.52,0.05,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
EPIC 202544292 20260420.4279 10.52CV 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 6030504279739666176,2461150.9279,10.66,0.05,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
Gaia DR3 6030504279739666176 20260420.4279 10.66CV 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
ASAS J165452-3322.0,2461150.9279,10.80,0.05,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
ASAS J165452-3322.0 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5980717637399865088,2461150.9279,10.71,0.05,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 5980717637399865088 20260420.4279 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
Gaia DR3 5970483383094628480,2461150.9279,10.97,0.05,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
Gaia DR3 5970483383094628480 20260420.4279 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
Gaia DR3 5977022213087774720,2461150.9279,10.97,0.05,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
Gaia DR3 5977022213087774720 20260420.4279 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
Gaia DR3 5979908254988656256,2461150.9279,11.02,0.05,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
Gaia DR3 5979908254988656256 20260420.4279 11.02CV 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
Gaia DR3 6020736424591264640,2461150.9279,10.80,0.05,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
Gaia DR3 6020736424591264640 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5972720098986394368,2461150.9279,11.03,0.05,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
Gaia DR3 5972720098986394368 20260420.4279 11.03CV 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
Gaia DR3 6031776311590949120,2461150.9279,10.60,0.05,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 6031776311590949120 20260420.4279 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202646460,2461150.9279,10.47,0.05,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
EPIC 202646460 20260420.4279 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029815882453093760,2461150.9279,10.65,0.05,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
Gaia DR3 6029815882453093760 20260420.4279 10.65CV 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
Gaia DR3 6029805741929182208,2461150.9279,10.63,0.05,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
Gaia DR3 6029805741929182208 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6027984061662492288,2461150.9279,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6027984061662492288 20260420.4279 10.72CV 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
Gaia DR3 5979193611093616256,2461150.9279,10.78,0.05,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
Gaia DR3 5979193611093616256 20260420.4279 10.78CV 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
Gaia DR3 5978767339884525696,2461150.9279,11.04,0.05,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
Gaia DR3 5978767339884525696 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5970551479755465984,2461150.9279,11.10,0.05,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
Gaia DR3 5970551479755465984 20260420.4279 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6024930065000138880,2461150.9279,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6024930065000138880 20260420.4279 10.72CV 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 J160828-2905.1,2461150.9279,10.62,0.05,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
ASAS J160828-2905.1 20260420.4279 10.62CV 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
ASAS J170120-3833.8,2461150.9279,11.20,0.05,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
ASAS J170120-3833.8 20260420.4279 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9279,10.68,0.05,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
VARIABLE_NAME 20260420.4279 10.68CV 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
Gaia DR3 5980326829732923520,2461150.9279,10.89,0.05,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 5980326829732923520 20260420.4279 10.89CV 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
ASASSN-V J170851.99-313120.3,2461150.9279,10.64,0.05,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 J170851.99-313120.3 20260420.4279 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978765523128819328,2461150.9279,10.99,0.05,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
Gaia DR3 5978765523128819328 20260420.4279 10.99CV 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 6043868740469671168,2461150.9279,10.74,0.05,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 6043868740469671168 20260420.4279 10.74CV 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
Gaia DR3 6028953074975941888,2461150.9279,10.92,0.05,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
Gaia DR3 6028953074975941888 20260420.4279 10.92CV 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
Gaia DR3 5978817676902050304,2461150.9279,11.07,0.05,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 5978817676902050304 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980004844548539264,2461150.9279,10.93,0.05,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 5980004844548539264 20260420.4279 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6028045977914500992,2461150.9279,10.74,0.05,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 6028045977914500992 20260420.4279 10.74CV 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 J160828-2905.1,2461150.9279,10.55,0.05,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
ASAS J160828-2905.1 20260420.4279 10.55CV 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
Gaia DR3 5978849704486886016,2461150.9279,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5978849704486886016 20260420.4279 10.73CV 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
Gaia DR3 6026802224126306560,2461150.9279,10.91,0.05,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 6026802224126306560 20260420.4279 10.91CV 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
ASAS J171838-3333.3,2461150.9279,11.03,0.05,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 J171838-3333.3 20260420.4279 11.03CV 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
Gaia DR3 5978782698682321536,2461150.9279,10.89,0.05,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 5978782698682321536 20260420.4279 10.89CV 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
Gaia DR3 5980674855118388224,2461150.9279,10.93,0.05,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 5980674855118388224 20260420.4279 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6023688682022234880,2461150.9279,10.89,0.05,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 6023688682022234880 20260420.4279 10.89CV 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
Gaia DR3 5977830629039893504,2461150.9279,11.00,0.05,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
Gaia DR3 5977830629039893504 20260420.4279 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4107301693650025344,2461150.9279,10.89,0.05,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 4107301693650025344 20260420.4279 10.89CV 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
OGLE-BLG-ECL-001057,2461150.9279,10.87,0.05,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
OGLE-BLG-ECL-001057 20260420.4279 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J170210.35-294954.8,2461150.9279,10.86,0.05,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
ASASSN-V J170210.35-294954.8 20260420.4279 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
Gaia DR3 5976704552989942144,2461150.9279,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5976704552989942144 20260420.4279 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6026697667434210304,2461150.9279,10.94,0.05,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
Gaia DR3 6026697667434210304 20260420.4279 10.94CV 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
[HHR2012] J171421.1-362603,2461150.9279,11.08,0.05,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
[HHR2012] J171421.1-362603 20260420.4279 11.08CV 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
Gaia DR3 5980370707089668352,2461150.9279,10.94,0.05,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
Gaia DR3 5980370707089668352 20260420.4279 10.94CV 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
Gaia DR3 6026384680213811712,2461150.9279,10.99,0.05,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
Gaia DR3 6026384680213811712 20260420.4279 10.99CV 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 6026086373339804416,2461150.9279,11.01,0.05,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
Gaia DR3 6026086373339804416 20260420.4279 11.01CV 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
Gaia DR3 6026904955379861504,2461150.9279,11.01,0.05,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
Gaia DR3 6026904955379861504 20260420.4279 11.01CV 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
Gaia DR3 6027663377881630720,2461150.9279,10.99,0.05,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
Gaia DR3 6027663377881630720 20260420.4279 10.99CV 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 5975495403733683584,2461150.9279,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5975495403733683584 20260420.4279 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5979666023282285696,2461150.9279,11.10,0.05,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
Gaia DR3 5979666023282285696 20260420.4279 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6024555780060312704,2461150.9279,10.82,0.05,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
Gaia DR3 6024555780060312704 20260420.4279 10.82CV 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
Gaia DR3 5977053029453537920,2461150.9279,11.10,0.05,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
Gaia DR3 5977053029453537920 20260420.4279 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6026650766446353408,2461150.9279,10.95,0.05,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 6026650766446353408 20260420.4279 10.95CV 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
Gaia DR3 6028595218394860288,2461150.9279,10.87,0.05,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 6028595218394860288 20260420.4279 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4059168647959812864,2461150.9279,10.93,0.05,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 4059168647959812864 20260420.4279 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5972658217085009792,2461150.9279,11.22,0.05,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
Gaia DR3 5972658217085009792 20260420.4279 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
Gaia DR3 5979194676239042816,2461150.9279,10.95,0.05,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 5979194676239042816 20260420.4279 10.95CV 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
Gaia DR3 6032717699740371712,2461150.9279,10.86,0.05,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
Gaia DR3 6032717699740371712 20260420.4279 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
Gaia DR3 5980363216664980096,2461150.9279,10.97,0.05,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
Gaia DR3 5980363216664980096 20260420.4279 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
Gaia DR3 6044010199511785472,2461150.9279,10.80,0.05,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
Gaia DR3 6044010199511785472 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5980361013262868224,2461150.9279,10.95,0.05,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 5980361013262868224 20260420.4279 10.95CV 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
Gaia DR3 5978121999580831360,2461150.9279,11.12,0.05,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 5978121999580831360 20260420.4279 11.12CV 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 5980024429611435776,2461150.9279,10.94,0.05,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
Gaia DR3 5980024429611435776 20260420.4279 10.94CV 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
Gaia DR3 5970527123059274880,2461150.9279,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5970527123059274880 20260420.4279 11.17CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5975544435080841728,2461150.9279,11.20,0.05,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
Gaia DR3 5975544435080841728 20260420.4279 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6026568401778095872,2461150.9279,10.96,0.05,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 6026568401778095872 20260420.4279 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
Gaia DR3 5970551479755465984,2461150.9279,11.33,0.05,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
Gaia DR3 5970551479755465984 20260420.4279 11.33CV 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 J161821.57-303335.9,2461150.9279,10.78,0.05,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 J161821.57-303335.9 20260420.4279 10.78CV 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
Gaia DR3 6029797843586380160,2461150.9279,10.96,0.05,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 6029797843586380160 20260420.4279 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
Gaia DR3 5979930421442681344,2461150.9279,11.05,0.05,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 5979930421442681344 20260420.4279 11.05CV 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 6024586776864593408,2461150.9279,10.90,0.05,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 6024586776864593408 20260420.4279 10.90CV 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
ATO J246.9004-28.9305,2461150.9279,10.70,0.05,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
ATO J246.9004-28.9305 20260420.4279 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5979445944708523520,2461150.9279,11.02,0.05,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
Gaia DR3 5979445944708523520 20260420.4279 11.02CV 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
ASASSN-V J161642.50-302138.7,2461150.9279,10.83,0.05,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 J161642.50-302138.7 20260420.4279 10.83CV 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
Gaia DR3 5967265284325739904,2461150.9279,11.18,0.05,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
Gaia DR3 5967265284325739904 20260420.4279 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
Gaia DR3 5970537259122406016,2461150.9279,11.39,0.05,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 5970537259122406016 20260420.4279 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 5972648935633646976,2461150.9279,11.49,0.05,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 5972648935633646976 20260420.4279 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6025505831144819584,2461150.9279,10.88,0.05,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
Gaia DR3 6025505831144819584 20260420.4279 10.88CV 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
Gaia DR3 5970275158739425280,2461150.9279,11.36,0.05,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
Gaia DR3 5970275158739425280 20260420.4279 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980751687928619008,2461150.9279,11.06,0.05,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
Gaia DR3 5980751687928619008 20260420.4279 11.06CV 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
Gaia DR3 6028658165444435968,2461150.9279,10.90,0.05,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 6028658165444435968 20260420.4279 10.90CV 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
Gaia DR3 5980366648263901952,2461150.9279,10.91,0.05,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 5980366648263901952 20260420.4279 10.91CV 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
Gaia DR3 6019200063269961600,2461150.9279,11.23,0.05,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 6019200063269961600 20260420.4279 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 6029356939328786944,2461150.9279,11.05,0.05,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 6029356939328786944 20260420.4279 11.05CV 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 J170308.41-291253.0,2461150.9279,11.01,0.05,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 J170308.41-291253.0 20260420.4279 11.01CV 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
Gaia DR3 5979828854029821824,2461150.9279,11.29,0.05,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
Gaia DR3 5979828854029821824 20260420.4279 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980493538776781056,2461150.9279,10.97,0.05,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
Gaia DR3 5980493538776781056 20260420.4279 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
Gaia DR3 6024809015641665920,2461150.9279,11.01,0.05,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
Gaia DR3 6024809015641665920 20260420.4279 11.01CV 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
Gaia DR3 6026797688616593792,2461150.9279,11.12,0.05,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 6026797688616593792 20260420.4279 11.12CV 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 6031155706026870656,2461150.9279,10.94,0.05,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
Gaia DR3 6031155706026870656 20260420.4279 10.94CV 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
Gaia DR3 5980757322865785984,2461150.9279,11.07,0.05,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 5980757322865785984 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973345201362616192,2461150.9279,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5973345201362616192 20260420.4279 11.32CV 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
Gaia DR3 6021194611695420672,2461150.9279,11.09,0.05,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
Gaia DR3 6021194611695420672 20260420.4279 11.09CV 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
Gaia DR3 6021166574159883648,2461150.9279,11.07,0.05,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 6021166574159883648 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029441391264872960,2461150.9279,11.07,0.05,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 6029441391264872960 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029638483089790336,2461150.9279,10.97,0.05,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
Gaia DR3 6029638483089790336 20260420.4279 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
ASAS J171005-2934.8,2461150.9279,10.93,0.05,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
ASAS J171005-2934.8 20260420.4279 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6028822611136397440,2461150.9279,11.16,0.05,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
Gaia DR3 6028822611136397440 20260420.4279 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038903449034106368,2461150.9279,10.88,0.05,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
Gaia DR3 6038903449034106368 20260420.4279 10.88CV 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
EPIC 202673190,2461150.9279,10.82,0.05,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
EPIC 202673190 20260420.4279 10.82CV 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
Gaia DR3 6024422537309844224,2461150.9279,11.09,0.05,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
Gaia DR3 6024422537309844224 20260420.4279 11.09CV 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
Gaia DR3 6038682584638395776,2461150.9279,10.68,0.05,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
Gaia DR3 6038682584638395776 20260420.4279 10.68CV 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
Gaia DR3 5979908254988656256,2461150.9279,11.09,0.05,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
Gaia DR3 5979908254988656256 20260420.4279 11.09CV 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
Gaia DR3 5972719961547432320,2461150.9279,11.52,0.05,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
Gaia DR3 5972719961547432320 20260420.4279 11.52CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.06 17:16:49.50 -33:23:00.6
352.90238 2.70821 galactic Sco Second-epoch detections are separated by 1.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5979014631218487168 | 17:16:49.95 -33:23:10.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5979014631218487168,2461150.9279,11.06,0.05,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
Large-amplitude variable Gaia DR2 5979014631218487168 20260420.4279 11.06CV 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
Gaia DR3 6028180187140851712,2461150.9279,11.23,0.05,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 6028180187140851712 20260420.4279 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 6031870354191590656,2461150.9279,10.94,0.05,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
Gaia DR3 6031870354191590656 20260420.4279 10.94CV 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
Gaia DR3 5977643918243086336,2461150.9279,11.27,0.05,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
Gaia DR3 5977643918243086336 20260420.4279 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
Gaia DR3 6021270959039670016,2461150.9279,11.22,0.05,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
Gaia DR3 6021270959039670016 20260420.4279 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
Gaia DR3 6020632795614714752,2461150.9279,11.16,0.05,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
Gaia DR3 6020632795614714752 20260420.4279 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980014499711458176,2461150.9279,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5980014499711458176 20260420.4279 11.19CV 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
Gaia DR3 6021148913254229760,2461150.9279,11.22,0.05,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
Gaia DR3 6021148913254229760 20260420.4279 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
Gaia DR3 5979609673222247552,2461150.9279,11.29,0.05,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
Gaia DR3 5979609673222247552 20260420.4279 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6026539715741958144,2461150.9279,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6026539715741958144 20260420.4279 11.19CV 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
Gaia DR3 5978897808186722304,2461150.9279,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5978897808186722304 20260420.4279 11.32CV 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
Gaia DR3 6037585031520755840,2461150.9279,10.96,0.05,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 6037585031520755840 20260420.4279 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
Gaia DR3 6029091853964152064,2461150.9279,11.04,0.05,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
Gaia DR3 6029091853964152064 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6024809015641665920,2461150.9279,11.09,0.05,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
Gaia DR3 6024809015641665920 20260420.4279 11.09CV 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
Gaia DR3 6028695617471335424,2461150.9279,11.24,0.05,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
Gaia DR3 6028695617471335424 20260420.4279 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5972696214628053632,2461150.9279,11.56,0.05,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 5972696214628053632 20260420.4279 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5977052037342483456,2461150.9279,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5977052037342483456 20260420.4279 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5972650928496193536,2461150.9279,11.54,0.05,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
Gaia DR3 5972650928496193536 20260420.4279 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
Gaia DR3 5978351831961923456,2461150.9279,11.27,0.05,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
Gaia DR3 5978351831961923456 20260420.4279 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
Gaia DR3 6026614448129327744,2461150.9279,11.26,0.05,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
Gaia DR3 6026614448129327744 20260420.4279 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
Gaia DR3 5980471174940948992,2461150.9279,11.16,0.05,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
Gaia DR3 5980471174940948992 20260420.4279 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6023837116097382528,2461150.9279,11.31,0.05,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
Gaia DR3 6023837116097382528 20260420.4279 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 5979045722483091968,2461150.9279,11.49,0.05,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 5979045722483091968 20260420.4279 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978917491943857152,2461150.9279,11.33,0.05,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
Gaia DR3 5978917491943857152 20260420.4279 11.33CV 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
Gaia DR3 6026726186022172544,2461150.9279,11.46,0.05,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
Gaia DR3 6026726186022172544 20260420.4279 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
Gaia DR3 6025447831903746688,2461150.9279,11.20,0.05,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
Gaia DR3 6025447831903746688 20260420.4279 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5972689686279683456,2461150.9279,11.63,0.05,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
Gaia DR3 5972689686279683456 20260420.4279 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
Gaia DR3 6026291569634988928,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6026291569634988928 20260420.4279 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6025398422598686720,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6025398422598686720 20260420.4279 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5967196702285629056,2461150.9279,11.57,0.05,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 5967196702285629056 20260420.4279 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 6024774312305105280,2461150.9279,11.35,0.05,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
Gaia DR3 6024774312305105280 20260420.4279 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5973077543298666240,2461150.9279,11.70,0.05,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
Gaia DR3 5973077543298666240 20260420.4279 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
Gaia DR3 6025253763785277568,2461150.9279,11.29,0.05,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
Gaia DR3 6025253763785277568 20260420.4279 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030044099726521984,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030044099726521984 20260420.4279 11.28CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.34 16:43:23.89 -31:49:42.9
349.80926 9.22655 galactic Sco Second-epoch detections are separated by 6.6" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6030479059653028992 | 16:43:25.57 -31:49:56.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6030479059653028992,2461150.9279,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6030479059653028992 20260420.4279 11.34CV 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 6043845474620771712,2461150.9279,11.03,0.05,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
Gaia DR3 6043845474620771712 20260420.4279 11.03CV 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
Gaia DR3 5972679210885496704,2461150.9279,11.85,0.05,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
Gaia DR3 5972679210885496704 20260420.4279 11.85CV 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 6026693853439653888,2461150.9279,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6026693853439653888 20260420.4279 11.32CV 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
Gaia DR3 5980537416161740672,2461150.9279,11.37,0.05,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
Gaia DR3 5980537416161740672 20260420.4279 11.37CV 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
Gaia DR3 5973021605667961472,2461150.9279,11.78,0.05,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
Gaia DR3 5973021605667961472 20260420.4279 11.78CV 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
Gaia DR3 5972642549051017088,2461150.9279,11.60,0.05,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 5972642549051017088 20260420.4279 11.60CV 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
Gaia DR3 6025335853513707264,2461150.9279,11.37,0.05,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
Gaia DR3 6025335853513707264 20260420.4279 11.37CV 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
Gaia DR3 5973077504640975232,2461150.9279,11.90,0.05,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
Gaia DR3 5973077504640975232 20260420.4279 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
Gaia DR3 5980355137753544704,2461150.9279,11.41,0.05,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
Gaia DR3 5980355137753544704 20260420.4279 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
Gaia DR3 5972315306930499840,2461150.9279,11.76,0.05,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
Gaia DR3 5972315306930499840 20260420.4279 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5980339405398922624,2461150.9279,11.53,0.05,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
Gaia DR3 5980339405398922624 20260420.4279 11.53CV 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
Gaia DR3 5972691099363380992,2461150.9279,11.67,0.05,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
Gaia DR3 5972691099363380992 20260420.4279 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
EPIC 202598419,2461150.9279,11.06,0.05,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
EPIC 202598419 20260420.4279 11.06CV 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
Gaia DR3 5973250127977350400,2461150.9279,11.69,0.05,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
Gaia DR3 5973250127977350400 20260420.4279 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
Gaia DR3 5972703945576641664,2461150.9279,11.95,0.05,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
Gaia DR3 5972703945576641664 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J162632.26-335116.8,2461150.9279,11.47,0.05,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 J162632.26-335116.8 20260420.4279 11.47CV 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
Gaia DR3 6027287692831153152,2461150.9279,11.51,0.05,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
Gaia DR3 6027287692831153152 20260420.4279 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5972692709935309184,2461150.9279,11.74,0.05,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 5972692709935309184 20260420.4279 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
ATO J243.0695-28.8953,2461150.9279,11.11,0.05,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
ATO J243.0695-28.8953 20260420.4279 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.66 16:57:47.71 -38:32:22.1
346.46221 2.70010 galactic Sco Second-epoch detections are separated by 8.7" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5970511072703141248 | 16:57:48.34 -38:32:49.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5970511072703141248,2461150.9279,11.66,0.05,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
Large-amplitude variable Gaia DR2 5970511072703141248 20260420.4279 11.66CV 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 5972707042284171008,2461150.9279,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5972707042284171008 20260420.4279 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
Gaia DR3 5972265412230329600,2461150.9279,11.79,0.05,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
Gaia DR3 5972265412230329600 20260420.4279 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6037671029635566464,2461150.9279,11.38,0.05,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 6037671029635566464 20260420.4279 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037996420663061376,2461150.9279,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6037996420663061376 20260420.4279 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J243.0695-28.8953,2461150.9279,11.24,0.05,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
ATO J243.0695-28.8953 20260420.4279 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044148737974024832,2461150.9279,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6044148737974024832 20260420.4279 11.32CV 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 J164616.80-361223.4,2461150.9279,11.62,0.05,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 J164616.80-361223.4 20260420.4279 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 21362,2461150.9279,11.86,0.05,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
NSV 21362 20260420.4279 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
Gaia DR3 5980054082146299776,2461150.9279,11.77,0.05,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
Gaia DR3 5980054082146299776 20260420.4279 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
V0880 Sco,2461150.9279,11.69,0.05,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
V0880 Sco 20260420.4279 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
Gaia DR3 5973119148647104768,2461150.9279,11.97,0.05,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
Gaia DR3 5973119148647104768 20260420.4279 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
OGLE-BLG-LPV-234649,2461150.9279,11.88,0.05,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
OGLE-BLG-LPV-234649 20260420.4279 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
Gaia DR3 6030766066572879616,2461150.9279,11.72,0.05,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
Gaia DR3 6030766066572879616 20260420.4279 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
Gaia DR3 5972316165924070528,2461150.9279,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5972316165924070528 20260420.4279 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027391802801913216,2461150.9279,11.82,0.05,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
Gaia DR3 6027391802801913216 20260420.4279 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
Gaia DR3 6024719882170435328,2461150.9279,11.96,0.05,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 6024719882170435328 20260420.4279 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
Gaia DR3 5976997194880964736,2461150.9279,11.07,0.05,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 5976997194880964736 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J244.2765-29.6976,2461150.9279,10.43,0.05,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
ATO J244.2765-29.6976 20260420.4279 10.43CV 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
Gaia DR3 5972645400910392064,2461150.9279,11.61,0.05,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
Gaia DR3 5972645400910392064 20260420.4279 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J244.2765-29.6976,2461150.9279,10.76,0.05,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
ATO J244.2765-29.6976 20260420.4279 10.76CV 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 DR3 5977001833442895744,2461150.9279,10.46,0.05,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 5977001833442895744 20260420.4279 10.46CV 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 6026666739313257856,2461150.9279,11.21,0.05,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 6026666739313257856 20260420.4279 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
Gaia DR3 6024309352018329600,2461150.9279,11.63,0.05,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
Gaia DR3 6024309352018329600 20260420.4279 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
Gaia DR3 5970832649854186496,2461150.9279,11.26,0.05,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
Gaia DR3 5970832649854186496 20260420.4279 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
Gaia DR3 6028555498527230592,2461150.9279,10.80,0.05,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
Gaia DR3 6028555498527230592 20260420.4279 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5980674855112585600,2461150.9279,11.12,0.05,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 5980674855112585600 20260420.4279 11.12CV 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 5976507637327600512,2461150.9279,11.54,0.05,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
Gaia DR3 5976507637327600512 20260420.4279 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
ATO J253.2962-29.1276,2461150.9279,11.30,0.05,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 J253.2962-29.1276 20260420.4279 11.30CV 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 6038466805484167680,2461150.9279,11.39,0.05,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 6038466805484167680 20260420.4279 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 5979977803496434944,2461150.9279,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5979977803496434944 20260420.4279 10.73CV 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
Gaia DR3 5980575005712498688,2461150.9279,11.40,0.05,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
Gaia DR3 5980575005712498688 20260420.4279 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 5978996523675536128,2461150.9279,12.05,0.05,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
Gaia DR3 5978996523675536128 20260420.4279 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
Gaia DR3 5979511851017250688,2461150.9279,10.30,0.05,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
Gaia DR3 5979511851017250688 20260420.4279 10.30CV 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
V0901 Sco,2461150.9279,10.23,0.05,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
V0901 Sco 20260420.4279 10.23CV 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
VARIABLE_NAME,2461150.9279,10.90,0.05,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
VARIABLE_NAME 20260420.4279 10.90CV 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 J164916.47-292913.0,2461150.9279,10.38,0.05,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
ASASSN-V J164916.47-292913.0 20260420.4279 10.38CV 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 J160849.97-283552.8,2461150.9279,11.60,0.05,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
ASASSN-V J160849.97-283552.8 20260420.4279 11.60CV 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
Gaia DR3 6037509298350592384,2461150.9279,11.37,0.05,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
Gaia DR3 6037509298350592384 20260420.4279 11.37CV 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
Gaia DR3 6037089048694855424,2461150.9279,11.34,0.05,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
Gaia DR3 6037089048694855424 20260420.4279 11.34CV 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 6038476288771972480,2461150.9279,10.79,0.05,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
Gaia DR3 6038476288771972480 20260420.4279 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.46 17:15:39.56 -30:04:49.2
355.46060 4.81933 galactic Oph Second-epoch detections are separated by 6.6" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4059239875760326656 | 17:15:40.53 -30:04:54.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4059239875760326656,2461150.9279,11.46,0.05,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
Large-amplitude variable Gaia DR2 4059239875760326656 20260420.4279 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
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 10.58 16:16:07.16 -31:53:46.7
345.78167 13.46405 galactic Sco Second-epoch detections are separated by 2.3" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6037360559349013504 | 16:16:05.77 -31:53:41.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6037360559349013504,2461150.9279,10.58,0.05,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
Large-amplitude variable Gaia DR2 6037360559349013504 20260420.4279 10.58CV 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
Gaia DR3 5978664883470276224,2461150.9279,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5978664883470276224 20260420.4279 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4107293511689698304,2461150.9279,10.58,0.05,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
Gaia DR3 4107293511689698304 20260420.4279 10.58CV 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
KR Sco,2461150.9279,9.80,0.05,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
KR Sco 20260420.4279 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5978266585430232960,2461150.9279,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5978266585430232960 20260420.4279 11.17CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6041752695978583424,2461150.9279,11.16,0.05,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
Gaia DR3 6041752695978583424 20260420.4279 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.10 17:00:05.35 -29:13:32.6
354.13701 8.05082 galactic Oph Second-epoch detections are separated by 2.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6029668307347745280 | 17:00:03.97 -29:13:28.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6029668307347745280,2461150.9279,11.10,0.05,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
Large-amplitude variable Gaia DR2 6029668307347745280 20260420.4279 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6024707482611750528,2461150.9279,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6024707482611750528 20260420.4279 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J160820.53-295443.9,2461150.9279,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J160820.53-295443.9 20260420.4279 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4279 2461150.9279 11.56 16:36:18.59 -34:36:04.9
346.70514 8.53408 galactic Sco Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6020725532554919936 | 16:36:18.59 -34:36:10.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6020725532554919936,2461150.9279,11.56,0.05,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
Large-amplitude variable Gaia DR2 6020725532554919936 20260420.4279 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6020686190651456000,2461150.9279,11.90,0.05,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
Gaia DR3 6020686190651456000 20260420.4279 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
Gaia DR3 5979401968540663424,2461150.9279,10.62,0.05,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 5979401968540663424 20260420.4279 10.62CV 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
Gaia DR3 6028930908626057472,2461150.9279,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6028930908626057472 20260420.4279 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V3892 Oph,2461150.9279,7.82,0.05,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
V3892 Oph 20260420.4279 7.82CV 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
Gaia DR3 5980352011016517248,2461150.9279,10.59,0.05,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
Gaia DR3 5980352011016517248 20260420.4279 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
Gaia DR3 5978988964533475200,2461150.9279,11.00,0.05,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
Gaia DR3 5978988964533475200 20260420.4279 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5976512413331229824,2461150.9279,11.43,0.05,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
Gaia DR3 5976512413331229824 20260420.4279 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
Gaia DR3 6037000915970112512,2461150.9279,11.26,0.05,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
Gaia DR3 6037000915970112512 20260420.4279 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
Gaia DR3 5980541371943816576,2461150.9279,10.41,0.05,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
Gaia DR3 5980541371943816576 20260420.4279 10.41CV 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
Gaia DR3 5979064521620547584,2461150.9279,10.69,0.05,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
Gaia DR3 5979064521620547584 20260420.4279 10.69CV 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
Gaia DR3 5980320846791790848,2461150.9279,11.07,0.05,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 5980320846791790848 20260420.4279 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037320461532197888,2461150.9279,10.53,0.05,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
Gaia DR3 6037320461532197888 20260420.4279 10.53CV 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
Gaia DR3 5980632764438978304,2461150.9279,11.21,0.05,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 5980632764438978304 20260420.4279 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
First image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Last image: 2461150.92826743 20.04.2026 10:16:32.306 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.59
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8006
Objects passed selection criteria: 7981
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 5375.75
Average stars matched: 5184.5 (96.4424 %)
Memory usage VmPeak: 113864 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:22:41 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: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
First image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Last image: 2461150.92826743 20.04.2026 10:16:32.306 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 718
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.25
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: 24 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): 85502
Objects passed selection criteria: 85318
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 54222
Average stars matched: 50941.5 (93.9499 %)
Memory usage VmPeak: 1855416 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:26:23 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/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461150.92753051
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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits exists and is non-empty
Saving wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits to local_wcs_cache/
'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits exists and is non-empty
Saving wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits to local_wcs_cache/
'wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits'
wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits (1st reference image)
verification OK: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Image size: 942.2'x628.0' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:44.386 -34:00:08.14 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Image size: 942.0'x628.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:48.187 -33:58:57.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:48.187 -33:58:57.85
Angular distance between the image centers 0.0235 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Image size: 942.0'x628.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:47.473 -33:59:52.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:47.473 -33:59:52.47
Angular distance between the image centers 0.0115 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 16:41:48.187 -33:58:57.85
Second-epoch second image center 16:41:47.473 -33:59:52.47
Angular distance between the image centers 0.01537 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/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits &> /tmp/tmp.yPP4H1fK2b
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits &> /tmp/tmp.YkvDapypgJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits &> /tmp/tmp.vpFTnHduSR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits &> /tmp/tmp.7G7JZiG7jG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
util/transients/transient_factory_test31.sh has not found non-empty wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
wait
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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
Found non-empty wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
The reference image (wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits) and catalog (wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat) found
'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat' -> 'wcsmag.cat'
Read 8448 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.2438 to 260.3527 deg, Dec -39.3236 to -28.2459 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 240.2438 to 260.3527 deg, Dec -39.3236 to -28.2459 deg
Loaded 13743 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): 6495 out of 6674 total matches.
Matched with Tycho-2 6674 out of 8448 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.646317
a=0.000000 b=1.000000 c=22.646317
From vast_summary.log: estimated ref. image limiting mag.: -8.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.06
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
2.4 pix Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
10.4 pix fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
10.6 pix fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Limiting magnitude estimates:
14.1 mag. Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
14.0 mag. Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
12.5 mag. fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
12.5 mag. fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.2 (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.yPP4H1fK2b (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=8448
Got 8448 stars (including 7867 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 8448 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 955 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits -region wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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.YkvDapypgJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=572, passed=8450
Got 8450 stars (including 7869 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 8450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8242 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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 956 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits -region wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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.vpFTnHduSR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=692, passed=2645
Got 2645 stars (including 1953 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat
util/solve_plate_with_UCAC5 got 2645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 2624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 2624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.78"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 2624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.65"
Excluding outliers - 952 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits -region wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.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.7G7JZiG7jG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=756, passed=2630
Got 2630 stars (including 1874 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat
util/solve_plate_with_UCAC5 got 2630 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 950 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(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 2617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.87"
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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 2616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.80"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 2616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.71"
Excluding outliers - 945 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_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits -region wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
Saving fully-calibrated image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits'
Preparing the HTML report for the field Sco-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out00971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20629.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 39s
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: 16s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20536_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20536_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20540_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20540_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20542_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20542_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20543_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20543_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20556_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20556_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:31.56 -38:47:37.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:22.51 -39:02:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20567_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20567_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20569_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20569_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20573_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20573_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20574_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20574_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20576_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20576_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:06.15 -38:55:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.59, MAG_FAINT_SEARCH_LIMIT=10.57)GAIADR2_OUTPUT=# 2.796 5972646431702487424 259.52494172099 -38.92393374672 9.4073 9.1464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20582_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20582_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:36.53 -38:24:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.55, MAG_FAINT_SEARCH_LIMIT=10.53)GAIADR2_OUTPUT=# 4.705 5973471993121421696 258.90084226712 -38.40777804505 9.2012 8.9255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20583_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20583_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20589_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20589_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20597_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20597_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20601_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20601_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20607_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20607_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20618_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20618_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20620_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20620_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:12.07 -39:05:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20623_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20623_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20628_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20628_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20629_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20629_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20648_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20648_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:44.52 -39:05:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20651_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20651_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:23.10 -38:51:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.24, MAG_FAINT_SEARCH_LIMIT=11.22)GAIADR2_OUTPUT=# 1.821 5972649661518030592 259.34684318903 -38.85706716303 9.9674 9.1888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20656_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20656_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:59.66 -38:55:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 3.181 5972644984258154496 259.49782584776 -38.92236951855 10.3962 10.0623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20677_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20677_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:26.21 -39:06:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00922_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 00922_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:51:51.70 -38:02:38.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02649_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 02649_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:36:22.69 -35:15:15.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01772_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 01772_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:03:32.20 -36:55:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20001_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20001_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:13:43.79 -38:30:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00971_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 00971_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02345_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 02345_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06998_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 06998_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08199_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 08199_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:51:09.62 -29:01:26.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03313_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 03313_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:50:08.18 -34:17:39.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02934_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 02934_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:31:23.28 -34:42:09.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04240_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 04240_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:57:10.95 -33:15:36.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00967_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 00967_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:52:19.65 -38:00:52.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 05319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:01:52.23 -32:08:39.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03480_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 03480_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:04:48.59 -34:07:19.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 56s
Prepared the HTML report for the field Sco-03-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 ####
16:54:33.21 -38:05:47.5
17:17:58.57 -35:50:15.3
17:14:32.20 -29:27:46.9
17:17:36.70 -34:34:47.8
17:15:19.44 -30:12:23.3
17:13:54.15 -37:48:17.3
17:04:28.99 -37:57:06.4
17:16:25.34 -31:17:02.7
16:39:18.32 -31:53:30.8
16:41:47.25 -31:25:36.9
16:34:10.45 -34:51:10.4
17:18:31.45 -38:27:12.5
17:04:34.88 -37:58:21.5
17:01:31.06 -30:44:51.4
17:16:53.94 -29:54:49.4
17:18:18.07 -37:59:00.5
17:13:08.50 -29:18:02.7
17:19:01.25 -38:48:51.7
17:17:38.99 -29:47:13.0
17:18:16.05 -29:22:22.6
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/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits exists and is non-empty
wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits exists and is non-empty
wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits exists and is non-empty
wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits (1st reference image)
verification OK: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Image size: 942.2'x628.0' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:44.386 -34:00:08.14 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Image size: 942.0'x628.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:48.187 -33:58:57.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:48.187 -33:58:57.85
Angular distance between the image centers 0.0235 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Image size: 942.0'x628.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:41:47.473 -33:59:52.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:47.473 -33:59:52.47
Angular distance between the image centers 0.0115 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 16:41:48.187 -33:58:57.85
Second-epoch second image center 16:41:47.473 -33:59:52.47
Angular distance between the image centers 0.01537 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/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits &> /tmp/tmp.QovESR4m2n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits &> /tmp/tmp.L6aSuJVfW3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits &> /tmp/tmp.Moyz31k2G7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits &> /tmp/tmp.q9ea9cvR2p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
Found non-empty wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
The reference image (wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits) and catalog (wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat) found
'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat' -> 'wcsmag.cat'
Read 94880 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.1952 to 260.3527 deg, Dec -39.3356 to -28.2336 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 240.1952 to 260.3527 deg, Dec -39.3356 to -28.2336 deg
Loaded 13805 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): 9915 out of 11104 total matches.
Matched with Tycho-2 11104 out of 94880 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.395234
a=0.000000 b=1.000000 c=22.395234
From vast_summary.log: estimated ref. image limiting mag.: -8.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 604 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
2.2 pix Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
5.1 pix fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
4.8 pix fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Limiting magnitude estimates:
14.1 mag. Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
14.1 mag. Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
12.5 mag. fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
12.6 mag. fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QovESR4m2n (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=5626, passed=94876
Got 94876 stars (including 89092 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 94876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92905 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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 92905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 92887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 958 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits -region wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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.L6aSuJVfW3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=4, blended=5558, passed=95128
Got 95128 stars (including 89424 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 95128 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 92937 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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits -region wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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.Moyz31k2G7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=5547, passed=15896
Got 15896 stars (including 10342 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat
util/solve_plate_with_UCAC5 got 15896 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 15723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.62"
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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 15724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.61"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 15729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.47"
Excluding outliers - 951 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits -region wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.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.q9ea9cvR2p (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5884, passed=16092
Got 16092 stars (including 10193 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat
util/solve_plate_with_UCAC5 got 16092 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 15929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.65"
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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 15930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.64"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 15935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.50"
Excluding outliers - 948 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits -region wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.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_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_Sco-03-Q1b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Saving fully-calibrated image wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_Sco-03-Q1b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.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_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-15-28_20.00sec_-4.90C_LIGHTs_0012.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.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_2026-04-20_CI_Sco-03-Q1b1x1_051728_TTUQ1b1x1_1790600_kUELGDoC/wcs_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013.fits
Preparing the HTML report for the field Sco-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out105229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out115974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94494.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 495s
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: 329s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114939_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114939_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114946_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114946_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114953_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114953_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114957_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114957_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:52:18.03 -32:22:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.263 6027532712138225280 253.07406695923 -32.38029211703 11.1121 10.4207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114958_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114958_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114959_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114959_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114961_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114961_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:42:29.06 -36:18:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.490 6019546306329551104 250.62110348021 -36.30267044644 10.9850 9.9636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114962_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114962_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114964_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114964_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114974_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114974_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114978_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114978_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114979_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114979_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:32:29.44 -33:48:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 5.371 6023832649331340288 248.12095453469 -33.80938421177 10.6463 9.6981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114982_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114982_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114991_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114991_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114994_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114994_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114996_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 114996_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114997_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 114997_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:34:33.58 -35:05:08.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115010_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115010_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115012_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115012_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115015_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115015_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:09:08.89 -29:12:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.222 6041641473501153792 242.28671729531 -29.20602041842 11.7258 11.1728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115017_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115017_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115019_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115019_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:08:52.56 -29:10:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 2.737 6041642435585132416 242.21818412102 -29.17887319664 11.4883 10.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115020_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115020_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115023_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115023_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115024_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115024_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115025_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115025_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115026_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115026_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115030_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115030_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115039_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115039_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:15:28.63 -30:07:58.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115051_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115051_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:09:48.82 -29:17:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 3.843 6041626625795204736 242.45285183803 -29.28846957405 11.2122 10.2809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115054_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115054_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115056_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115056_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115057_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115057_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115061_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115061_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115066_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115066_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115067_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115067_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115071_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115071_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115073_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115073_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115074_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115074_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115075_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115075_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115076_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115076_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115077_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115077_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115081_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115081_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115083_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115083_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115084_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115084_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115086_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115086_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115092_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115092_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:39:26.44 -35:32:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.867 6020393823627965440 249.86002403247 -35.54443216196 10.5715 9.6355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115095_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115095_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:14:05.61 -32:09:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 1.364 6035862234238714112 243.52373673331 -32.16047153056 10.8218 9.9156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115097_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115097_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:22:48.97 -31:08:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 5.183 6037285414598058240 245.70236017745 -31.14198832758 10.8121 10.0895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115098_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115098_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115099_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115099_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:12:08.75 -36:14:35.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115103_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115103_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115104_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115104_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115122_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115122_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115125_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115125_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115128_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115128_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115129_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115129_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115131_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115131_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:11:07.93 -38:46:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 3.387 5973120355548732032 257.78421701531 -38.77776852945 10.8124 9.9156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115133_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115133_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:16.80 -33:17:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 5.715 5979019166744013184 259.06937649665 -33.29791631216 10.9772 10.6212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115134_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115134_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115135_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115135_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115141_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115141_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115143_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115143_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115145_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115145_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115150_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115150_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115151_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115151_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115154_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115154_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:23:10.26 -29:41:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 0.175 6038083556956453632 245.79280513429 -29.68576955587 10.7056 9.7232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115156_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115156_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115157_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115157_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:33:26.46 -30:08:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 1.724 6031780331680389888 248.35973455695 -30.14410269858 10.4948 9.9604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115159_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115159_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115163_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115163_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115166_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115166_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:11:40.12 -36:52:24.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115167_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115167_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115168_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115168_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:14:04.16 -35:09:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 5.274 5978601691577058304 258.51904544813 -35.15190123906 9.8351 8.5985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115173_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115173_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:04.56 -34:40:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.680 5978645053570094848 259.02056181100 -34.66788417969 9.9845 8.5499 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115177_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115177_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115178_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115178_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115182_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115182_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115183_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115183_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115186_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115186_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:10:58.25 -30:16:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 5.016 6028842814669708928 257.74423210510 -30.27412516900 9.9058 8.7076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115187_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115187_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115188_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115188_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:09.30 -38:13:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.414 5973488966834324480 258.78999300092 -38.22849139762 10.5535 9.3314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115189_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115189_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115192_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115192_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115193_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115193_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:43.74 -33:58:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 5.128 5978959960573344896 258.93277381631 -33.97450455898 10.9645 10.4819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115201_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115201_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115203_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115203_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:12:14.17 -34:03:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.633 5978919179951119872 258.05992174899 -34.05066411673 9.9593 8.8513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115207_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115207_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115208_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115208_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115209_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115209_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115211_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115211_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115212_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115212_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115213_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115213_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115214_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115214_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115218_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115218_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115219_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115219_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115220_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115220_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115221_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115221_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115224_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115224_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115226_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115226_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:52:37.33 -31:57:54.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115229_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115229_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:03.38 -35:35:38.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115231_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115231_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115233_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115233_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115234_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115234_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115235_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115235_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115237_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115237_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115239_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115239_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115241_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115241_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115250_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115250_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:14:25.69 -33:13:51.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115252_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115252_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115254_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115254_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115257_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115257_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115261_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115261_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115263_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115263_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115265_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115265_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115266_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115266_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:10:38.04 -32:24:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 4.111 5980088682358982016 257.65982099156 -32.40899524568 9.3010 7.9854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115270_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115270_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115277_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115277_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115279_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115279_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115283_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115283_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:10:20.02 -30:23:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 3.557 6028747878693962240 257.58432646627 -30.39476066925 10.4553 9.9907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115289_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115289_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115291_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115291_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115294_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115294_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115295_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115295_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115296_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115296_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115297_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115297_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:05:04.52 -34:45:35.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115298_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115298_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115301_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115301_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:09:00.44 -38:01:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 5.172 5973401104656930944 257.25032550792 -38.01966435418 10.5437 9.6057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115304_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115304_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115305_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115305_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115307_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115307_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115308_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115308_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115309_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115309_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115316_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115316_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115317_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115317_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115320_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115320_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115322_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115322_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115324_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115324_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115326_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115326_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115330_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115330_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115334_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115334_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115335_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115335_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115336_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115336_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115338_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115338_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115340_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115340_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115344_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115344_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115348_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115348_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115351_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115351_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:18:18.02 -28:36:54.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115352_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115352_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:12:16.14 -28:25:04.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115364_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115364_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:10:36.76 -28:19:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.31, MAG_FAINT_SEARCH_LIMIT=9.29)GAIADR2_OUTPUT=# 3.220 6041838698405416704 242.65225397331 -28.33132923313 8.8872 8.1178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115367_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115367_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:48.24 -29:11:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.72, MAG_FAINT_SEARCH_LIMIT=9.70)GAIADR2_OUTPUT=# 4.366 4107344059219571072 258.95203445811 -29.18596833002 8.0738 6.8159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115369_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115369_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115371_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115371_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:08:54.56 -28:21:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.57, MAG_FAINT_SEARCH_LIMIT=9.55)GAIADR2_OUTPUT=# 1.468 6041824640969220608 242.22759401187 -28.36369060659 9.3223 8.8779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115382_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115382_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:54.76 -29:54:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.24, MAG_FAINT_SEARCH_LIMIT=10.22)GAIADR2_OUTPUT=# 3.912 4059237814212851968 259.22890522906 -29.91084424559 9.0936 8.1542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115392_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115392_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115400_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115400_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:18:12.70 -28:34:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.22, MAG_FAINT_SEARCH_LIMIT=10.20)GAIADR2_OUTPUT=# 0.323 6039096756923697280 244.55282457523 -28.57648913709 9.5015 8.7035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115401_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115401_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:39:18.37 -31:53:31.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115407_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115407_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:15.88 -29:22:24.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115411_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115411_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115421_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115421_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:10:14.49 -28:21:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.48, MAG_FAINT_SEARCH_LIMIT=10.46)GAIADR2_OUTPUT=# 2.988 6041833510085084288 242.56000666865 -28.35681920900 10.1237 9.3950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115422_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115422_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115424_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115424_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:19:00.74 -38:48:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 3.190 5972660411778306304 259.75217317456 -38.81424630159 10.1052 9.0574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115429_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115429_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:34:10.42 -34:51:09.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115430_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115430_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115438_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115438_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115439_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115439_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115440_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115440_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:39.10 -29:14:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.90, MAG_FAINT_SEARCH_LIMIT=10.88)GAIADR2_OUTPUT=# 0.362 4107424804635982848 259.41280570149 -29.23619365060 10.3313 9.9596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115441_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115441_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:59.65 -38:55:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.28, MAG_FAINT_SEARCH_LIMIT=11.26)GAIADR2_OUTPUT=# 2.811 5972644984258154496 259.49782584776 -38.92236951855 10.3962 10.0623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115448_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115448_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115451_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115451_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115457_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115457_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115469_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115469_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115473_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115473_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:26.27 -39:06:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115474_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115474_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115476_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115476_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115481_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115481_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:10:32.57 -28:29:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 3.923 6041827772008732416 242.63501387385 -28.49220837676 10.1172 9.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115485_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115485_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115488_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115488_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115490_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115490_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115493_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115493_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115496_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115496_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115510_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115510_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115511_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115511_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115512_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115512_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115520_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115520_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115521_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115521_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115526_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115526_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115528_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115528_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115530_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115530_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115531_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115531_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115532_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115532_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115533_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115533_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115535_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115535_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115538_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115538_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:55.20 -30:03:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 1.888 4059185411203478144 259.48023246930 -30.05131751734 10.5566 9.8535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115542_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115542_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115550_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115550_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:02.92 -39:07:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115551_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115551_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115556_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115556_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115564_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115564_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115567_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115567_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115570_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115570_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115573_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115573_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115579_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115579_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115585_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115585_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115592_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115592_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115593_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115593_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115597_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115597_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115598_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115598_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115599_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115599_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115600_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115600_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115614_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115614_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:56.68 -29:58:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 4.071 4059209398702715648 259.48626437231 -29.97379430384 10.7671 10.2199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115616_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115616_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115619_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115619_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115632_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115632_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115641_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115641_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115644_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115644_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115645_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115645_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115647_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115647_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115649_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115649_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115654_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115654_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115657_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115657_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115658_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115658_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115660_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115660_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115661_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115661_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115662_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115662_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115668_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115668_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115672_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115672_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115673_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115673_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115674_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115674_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115677_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115677_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115678_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115678_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115684_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115684_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115686_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115686_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115689_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115689_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115690_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115690_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115694_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115694_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115695_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115695_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115696_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115696_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115697_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115697_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115698_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115698_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115700_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115700_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115703_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115703_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115704_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115704_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115705_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115705_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115708_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115708_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:19:07.57 -34:35:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.67, MAG_FAINT_SEARCH_LIMIT=11.65)GAIADR2_OUTPUT=# 5.030 5978680929449682560 259.78323598720 -34.59494305814 10.2446 9.3751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115709_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115709_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115713_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115713_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115715_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115715_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:15:25.76 -28:27:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 3.407 6039156886466993280 243.85701783400 -28.46484521479 10.4629 9.4775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115717_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115717_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115718_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115718_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:09:53.05 -28:24:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 3.238 6041831620299227264 242.47071825083 -28.40770228071 11.0899 10.3809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115720_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115720_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115726_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115726_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115728_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115728_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115731_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115731_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115734_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115734_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115737_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115737_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115740_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115740_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115742_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115742_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:13:30.58 -29:23:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 4.345 4107361166005647872 258.37836928562 -29.39148474887 9.9481 8.7968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115743_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115743_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115744_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115744_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:19:18.37 -28:37:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 0.971 6038998007033448576 244.82684877934 -28.62999606659 10.7993 9.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115745_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115745_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115747_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115747_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:34.32 -38:58:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115748_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115748_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115752_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115752_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115753_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115753_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115755_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115755_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115756_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115756_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115761_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115761_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115762_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115762_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115765_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115765_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:14:43.39 -28:29:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.58, MAG_FAINT_SEARCH_LIMIT=11.56)GAIADR2_OUTPUT=# 4.523 6039145685186131584 243.67974577633 -28.48831013786 10.4018 9.1753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115768_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115768_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115769_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115769_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:11:30.54 -28:36:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 1.426 6041775648284266752 242.87688859214 -28.60634621892 11.1216 10.6024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115770_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115770_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115771_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115771_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115772_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115772_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115773_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115773_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:19:05.90 -38:46:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.748 5972660622267521152 259.77508966406 -38.77917984136 10.7637 9.7229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115774_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115774_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115777_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115777_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115779_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115779_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115781_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115781_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115784_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115784_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115785_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115785_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115787_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115787_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115789_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115789_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115792_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115792_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115799_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115799_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115800_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115800_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115801_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115801_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115803_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115803_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115805_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115805_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115806_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115806_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115811_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115811_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115813_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115813_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115816_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115816_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:16.62 -29:39:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 3.288 4059270249814419840 259.56921888662 -29.65432968876 11.0335 10.5401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115818_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115818_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115819_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115819_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115820_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115820_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115824_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115824_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115826_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115826_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115828_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115828_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:33.98 -38:59:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.076 5972633370666588928 259.64033198304 -38.98900382984 10.9963 10.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115835_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115835_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115836_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115836_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:12.97 -39:01:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115838_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115838_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115840_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115840_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115846_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115846_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115850_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115850_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115853_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115853_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115855_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115855_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115860_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115860_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115861_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115861_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115862_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115862_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115863_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115863_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115864_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115864_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115865_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115865_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:52.98 -38:50:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 2.839 5972658869920060544 259.72030536525 -38.83434696453 10.8826 9.7729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115870_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115870_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115874_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115874_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115879_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115879_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115881_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115881_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115883_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115883_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115885_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115885_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115886_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115886_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:05.11 -31:47:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 5.200 5980371561702545152 259.52292332004 -31.79426279857 10.6866 9.9505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115887_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115887_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115888_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115888_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115890_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115890_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115893_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115893_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115896_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115896_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115897_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115897_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:09:28.99 -28:25:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 1.213 6041843130811584768 242.37117480747 -28.42499483912 11.4902 10.9790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115898_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115898_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115900_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115900_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115902_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115902_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115904_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115904_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115909_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115909_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115910_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115910_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115913_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115913_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115914_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115914_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115916_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115916_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:55.04 -30:15:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 4.790 4059177856455672320 259.48082600243 -30.26569853365 10.6225 9.8019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115921_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115921_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:11.64 -29:38:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.953 4059277465362028544 259.29776598251 -29.64843234101 11.1576 10.6397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115922_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115922_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115923_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115923_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115924_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115924_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115925_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115925_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115926_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115926_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115930_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115930_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:33.44 -29:18:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 5.230 4107341001203180800 258.89096860563 -29.30344460068 10.8207 10.0303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115933_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115933_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115935_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115935_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115940_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115940_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115942_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115942_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:49.16 -30:22:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 4.180 4059159332162061696 259.45613053290 -30.36875306035 10.5967 9.7175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115943_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115943_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115944_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115944_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115945_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115945_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115946_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115946_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115947_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115947_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115951_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115951_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115953_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115953_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115954_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115954_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115955_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115955_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115956_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115956_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115958_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115958_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115960_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115960_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115962_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115962_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115963_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115963_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115966_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115966_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115970_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115970_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115971_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115971_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115972_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115972_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115973_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115973_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:55.98 -29:35:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 1.656 4059283203440902144 259.48371655746 -29.58714415176 10.7641 9.8186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115974_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115974_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:37.70 -31:00:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 4.009 5980484502162546432 259.40834448293 -31.00584284411 11.0564 10.8548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115977_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115977_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115979_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115979_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115981_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115981_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115982_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115982_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115986_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115986_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115990_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115990_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115991_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 115991_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:20.50 -39:03:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115994_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115994_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115995_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115995_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115996_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 115996_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116002_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116002_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116015_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116015_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116020_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116020_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:10:24.35 -28:34:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 3.993 6041825435546294400 242.60073418194 -28.56959143021 10.5295 9.2950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116022_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116022_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116026_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116026_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:11:53.09 -28:37:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 2.769 6041769532250813184 242.97033204339 -28.62356854846 11.0454 10.2600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116031_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116031_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116032_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116032_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:19:04.09 -38:50:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 3.621 5972658114006552960 259.76602882869 -38.84518152627 11.2605 10.8717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116034_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116034_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116038_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116038_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116040_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116040_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116042_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116042_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116048_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116048_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116049_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116049_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116052_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116052_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:15:21.75 -28:26:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.669 6039157161344902272 243.84025565876 -28.44528010668 10.8410 10.0063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116053_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116053_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116054_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116054_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116056_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116056_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116058_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116058_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116061_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116061_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116063_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116063_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116067_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116067_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:14:43.16 -39:04:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 4.971 5972321560374418560 258.67850171009 -39.06680679974 11.3908 10.8981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116069_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116069_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116074_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116074_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116075_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116075_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116076_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116076_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116078_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116078_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116079_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116079_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116081_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116081_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116090_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116090_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116092_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116092_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116094_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116094_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116095_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116095_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116096_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116096_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116097_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116097_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116098_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116098_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116102_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116102_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:15:13.65 -28:27:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 4.928 6039145307234876672 243.80578812031 -28.46157517981 10.8532 9.9156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116110_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116110_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116111_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116111_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116115_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116115_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116118_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116118_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116121_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116121_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:18:40.38 -28:36:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 0.615 6039186641995324928 244.66809543473 -28.60218711136 11.3796 10.8634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116124_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116124_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116129_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116129_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:04.94 -39:00:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 4.831 5972632752191299584 259.51886400343 -39.01415637161 11.2470 10.2958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116133_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116133_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116134_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116134_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116137_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116137_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116138_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116138_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:15:52.20 -28:35:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.964 6039151457628314496 243.96760441841 -28.59597391208 11.3131 10.6951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116140_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116140_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116142_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116142_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116143_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116143_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116147_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116147_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116148_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116148_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116149_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116149_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116156_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116156_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116159_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116159_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116161_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116161_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116163_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116163_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:11:04.31 -28:24:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 5.532 6041834231639386240 242.76730107927 -28.40910405733 10.7843 9.6358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116164_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116164_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116171_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116171_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:06.51 -38:28:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 4.816 5972727000952251776 259.52578380412 -38.47461534575 10.0949 8.5868 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116173_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116173_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116178_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116178_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116179_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116179_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:26.92 -38:59:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116183_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116183_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116188_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116188_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116190_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116190_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116199_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116199_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116201_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116201_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116211_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116211_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116213_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116213_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116215_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116215_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116227_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116227_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116234_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116234_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:56.26 -38:47:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 5.595 5972659213518246656 259.73277349548 -38.79656364765 11.3147 10.8643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116237_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116237_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116242_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116242_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116247_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116247_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116249_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116249_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116250_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116250_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116251_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116251_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:55.77 -30:56:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.451 5980491069263617792 259.48280667616 -30.93570916123 11.3402 10.5431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116253_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116253_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116256_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116256_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116257_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116257_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116261_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116261_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116268_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116268_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116269_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116269_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116274_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116274_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116275_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116275_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116279_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116279_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116280_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116280_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116290_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116290_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:46.10 -39:03:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116293_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116293_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116294_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116294_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:14:41.31 -29:16:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116296_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116296_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:11:11.44 -28:21:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 1.758 6041834953193900288 242.79767756552 -28.36120619158 11.5953 10.6956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116298_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116298_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116299_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116299_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116301_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116301_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116302_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116302_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116315_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116315_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116319_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116328_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116328_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116332_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116332_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116335_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116335_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116345_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116345_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:08:45.48 -28:18:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.716 6042012764841550080 242.18870881355 -28.30073443686 11.7193 10.9771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116347_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116347_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116349_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116349_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116351_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116351_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116359_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116359_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116367_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116367_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:12:44.08 -28:23:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.222 6042148378425120128 243.18376636319 -28.39241674516 11.9274 11.0513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116375_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116375_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116376_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116376_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116377_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116377_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116381_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116381_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116401_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116401_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116404_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116404_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116427_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116427_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:08:47.79 -28:15:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.387 6042013108438937600 242.19908590516 -28.26606063412 11.4300 10.6552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116430_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116430_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:22.00 -39:09:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 5.563 5972264763745669504 259.08991882488 -39.16022992480 11.7255 11.2588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116434_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116434_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116441_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116441_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116454_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116454_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116457_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116457_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:41:52.30 -32:23:04.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116468_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116468_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116478_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116478_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116485_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116485_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:34.22 -39:04:02.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116507_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116507_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116522_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116522_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116523_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116523_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116537_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116537_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116538_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116538_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116550_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116550_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116604_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 116604_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116609_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 116609_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77919_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 77919_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:11:02.21 -29:25:02.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86315_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 86315_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:19:33.02 -30:54:22.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78410_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 78410_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:24:40.18 -29:42:20.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35271_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 35271_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:04:48.65 -34:07:20.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44214_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 44214_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:57:10.91 -33:15:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 20278_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79222_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 79222_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 01123_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79179_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 79179_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19812_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 19812_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44992_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 44992_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 48107_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03225_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 03225_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68750_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 68750_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71103_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 71103_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75048_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 75048_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12643_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 12643_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86834_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 86834_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:46:28.14 -31:16:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52114_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 52114_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79644_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 79644_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 76560_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01862_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 01862_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72843_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 72843_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107500_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 107500_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73548_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 73548_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74870_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 74870_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94494_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 94494_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56227_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 56227_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51977_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 51977_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 53566_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86964_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 86964_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47277_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 47277_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56331_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 56331_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:14:32.20 -29:27:45.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14258_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 14258_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:03:32.19 -36:55:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106289_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 106289_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78196_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 78196_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67321_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 67321_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61381_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 61381_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105820_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 105820_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:08:54.60 -28:51:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 4.985 6041791689977714176 242.22762681893 -28.86484197861 12.0633 11.5258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105632_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 105632_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105229_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 105229_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:36.37 -33:54:56.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65547_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 65547_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63737_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 63737_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31150_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 31150_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53403_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 53403_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53182_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 53182_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38161_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 38161_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78807_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 78807_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30914_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 30914_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26372_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 26372_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46782_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 46782_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68366_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 68366_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79002_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 79002_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80988_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 80988_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72927_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 72927_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39731_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 39731_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13399_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 13399_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85638_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 85638_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72721_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 72721_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44384_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 44384_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91255_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 91255_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56064_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 56064_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:06:02.38 -29:28:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 87546_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70704_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
Preparing report for the candidate 70704_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 45191_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:41:45.31 -33:08:45.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32743_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 32743_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:50:08.15 -34:17:38.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24090_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 24090_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:36:22.65 -35:15:14.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27287_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 27287_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:31:23.29 -34:42:09.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11724_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 11724_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:39:04.92 -37:13:04.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41343_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 41343_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:55:57.89 -33:30:24.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20603_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 20603_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:00:36.94 -35:56:03.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07400_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 07400_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:52:19.67 -38:00:51.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07004_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 07004_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:51:51.71 -38:02:38.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60392_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 60392_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:14:11.70 -31:39:55.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03034_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 03034_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:35.37 -38:35:47.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73417_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 73417_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:01:52.31 -32:08:39.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21162_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 21162_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:16:21.09 -35:45:09.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68852_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 68852_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 16:56:37.67 -30:34:51.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06598_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 06598_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:03:51.02 -38:09:08.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26046_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 26046_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:18:59.50 -34:59:27.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94297_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 94297_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:12:58.51 -32:26:18.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80693_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 80693_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:51.36 -30:12:38.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40558_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 40558_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:15:19.01 -33:32:54.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68323_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 68323_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:08:47.52 -30:24:15.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74620_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013
The candidate 74620_fd_Sco-03-Q1b1x1_2026-04-20_05-16-32_20.00sec_-4.90C_LIGHTs_0013 did not pass the final checks
**** FOUND 17:17:03.18 -32:39:48.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 30s
make_report_in_HTML.sh TOTAL: 854s
Prepared the HTML report for the field Sco-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:54:33.21 -38:05:47.5
17:17:58.57 -35:50:15.3
17:14:32.20 -29:27:46.9
17:17:36.70 -34:34:47.8
17:15:19.44 -30:12:23.3
17:13:54.15 -37:48:17.3
17:04:28.99 -37:57:06.4
17:16:25.34 -31:17:02.7
16:39:18.32 -31:53:30.8
16:41:47.25 -31:25:36.9
16:34:10.45 -34:51:10.4
17:18:31.45 -38:27:12.5
17:04:34.88 -37:58:21.5
17:01:31.06 -30:44:51.4
17:16:53.94 -29:54:49.4
17:18:18.07 -37:59:00.5
17:13:08.50 -29:18:02.7
17:19:01.25 -38:48:51.7
17:17:38.99 -29:47:13.0
17:18:16.05 -29:22:22.6
17:17:31.77 -38:57:25.7
16:52:04.56 -38:46:18.0
17:14:39.76 -34:28:15.9
16:19:18.53 -32:29:03.2
17:17:11.38 -33:32:51.5
16:53:57.62 -30:38:59.6
16:44:25.07 -33:02:04.4
16:47:58.53 -35:08:30.4
16:59:49.57 -29:47:38.7
16:33:45.56 -32:35:47.4
16:20:46.44 -31:42:18.1
17:05:03.88 -35:01:09.1
16:39:29.03 -33:32:16.3
16:12:09.96 -31:20:03.5
17:00:03.64 -31:40:43.1
16:07:04.88 -31:10:44.2
16:19:38.37 -29:52:27.4
16:47:05.39 -36:04:39.3
16:38:57.39 -35:00:56.5
16:40:48.19 -32:42:11.0
16:54:36.98 -37:51:38.5
16:20:36.11 -32:17:42.0
17:15:49.22 -37:46:54.1
16:12:06.42 -31:44:16.0
16:38:42.80 -33:29:45.7
16:35:30.41 -33:47:05.2
16:49:36.21 -32:19:57.9
16:58:46.90 -35:25:52.6
16:54:42.27 -36:22:48.4
16:34:32.89 -34:01:30.6
16:10:12.44 -30:03:36.5
16:10:45.51 -30:21:54.4
16:35:46.88 -33:26:32.1
16:17:39.57 -32:18:55.5
16:10:04.39 -30:32:37.6
16:40:30.89 -37:11:57.4
16:08:07.11 -31:08:58.3
16:59:13.36 -29:36:15.5
17:11:40.66 -38:29:39.7
16:08:29.59 -30:30:05.6
16:48:47.59 -32:02:01.1
17:15:45.45 -32:40:17.9
16:06:31.09 -31:23:36.4
17:15:20.12 -34:44:38.1
16:55:53.04 -39:13:40.1
16:11:44.57 -29:32:08.6
16:34:43.50 -32:48:05.2
17:08:54.67 -33:06:40.2
16:08:30.31 -29:02:24.1
16:59:42.24 -29:43:44.1
16:57:04.19 -34:39:15.2
17:15:23.05 -34:30:14.9
17:13:56.70 -37:45:16.7
16:06:52.62 -31:18:49.5
17:14:32.29 -36:34:46.3
17:09:49.50 -30:16:59.6
16:55:54.10 -30:55:44.7
16:33:42.10 -32:28:30.2
17:09:12.12 -33:51:25.4
16:50:02.95 -32:25:41.0
17:14:55.87 -35:14:25.0
17:16:14.77 -31:40:34.2
16:08:14.47 -29:27:57.8
17:17:10.54 -38:18:35.5
17:14:33.67 -35:05:17.6
17:12:56.78 -36:19:47.3
17:08:38.56 -33:39:27.0
17:15:38.51 -38:41:20.7
16:24:05.18 -33:09:32.6
17:14:27.90 -38:23:13.9
17:13:45.71 -38:30:58.8
17:13:46.55 -38:11:23.4
17:04:56.93 -34:09:55.3
17:09:52.40 -31:23:07.5
17:06:36.52 -36:58:36.7
17:02:15.87 -29:35:17.9
17:18:54.90 -38:39:24.4
16:56:31.68 -38:02:14.6
17:04:17.68 -34:51:07.1
17:10:19.27 -36:58:43.6
17:15:52.98 -37:10:16.8
17:19:07.80 -37:44:49.2
17:18:09.76 -33:51:24.2
17:17:02.77 -39:07:28.3
17:17:17.85 -35:24:23.0
17:07:11.94 -37:29:54.4
17:14:27.24 -33:13:58.9
17:07:53.35 -38:28:22.7
17:18:28.67 -38:24:30.7
17:17:41.49 -37:21:08.4
17:18:56.40 -38:14:59.8
17:10:09.81 -34:45:07.0
17:17:43.41 -32:12:12.8
17:19:18.80 -37:18:39.6
17:16:44.85 -38:11:47.7
17:01:49.03 -39:17:06.0
17:16:26.99 -38:48:55.9
17:09:17.84 -36:40:48.3
17:17:53.85 -38:07:50.4
17:12:57.22 -38:27:39.7
17:18:08.44 -37:18:00.6
16:43:44.06 -33:09:04.5
16:45:14.29 -32:37:55.9
17:17:36.12 -34:34:48.1
17:10:19.76 -37:19:27.9
17:13:07.44 -29:17:51.5
17:11:46.36 -30:46:04.1
17:13:48.77 -31:28:34.7
17:09:57.39 -36:16:15.1
17:07:35.62 -37:23:12.6
17:16:00.43 -34:15:54.8
17:16:15.58 -31:28:19.6
17:12:06.86 -29:19:15.8
17:19:18.11 -38:18:12.0
17:17:18.08 -30:12:57.7
16:55:34.87 -30:46:13.8
17:16:08.50 -29:55:33.4
17:02:52.61 -35:07:36.9
17:16:15.11 -31:28:16.0
17:02:16.54 -31:09:52.9
16:09:21.33 -28:30:17.9
16:54:46.25 -33:52:12.8
17:18:52.49 -33:30:26.5
17:12:34.34 -29:51:02.2
17:09:27.44 -29:14:58.1
16:09:37.84 -28:19:20.5
17:03:57.16 -33:45:19.1
17:03:42.73 -37:10:09.8
16:56:59.41 -32:28:58.4
17:17:16.33 -34:14:59.8
16:13:45.17 -28:23:26.2
17:03:18.94 -29:32:30.4
16:46:53.92 -30:07:53.5
17:18:53.14 -32:15:51.0
16:59:06.66 -34:11:40.0
17:15:59.66 -36:43:10.3
17:10:37.80 -37:18:10.3
17:04:28.57 -38:02:43.6
16:55:59.64 -31:08:59.9
16:36:22.76 -31:28:14.4
16:54:27.43 -29:47:25.8
16:53:13.32 -36:14:14.2
16:52:04.64 -29:46:23.3
16:36:58.07 -30:57:11.1
16:30:10.43 -33:17:05.9
16:58:21.71 -32:42:10.4
17:12:52.47 -31:41:59.7
16:26:52.24 -29:16:57.4
16:45:32.01 -31:25:44.1
16:54:50.85 -33:22:43.8
17:13:23.06 -30:49:08.2
16:56:10.63 -38:19:46.4
17:13:37.51 -35:50:38.1
17:12:20.35 -32:31:29.0
16:35:15.24 -34:32:33.9
17:15:51.73 -38:29:22.1
16:34:45.34 -30:00:58.4
16:23:12.82 -28:53:21.9
17:04:06.40 -29:17:08.9
17:05:28.63 -29:20:22.6
16:53:28.33 -30:40:09.6
17:19:02.93 -33:18:48.5
17:16:18.46 -34:07:00.4
17:00:22.06 -37:59:01.4
16:25:47.25 -32:37:57.6
16:08:29.10 -29:05:14.9
17:01:18.19 -38:33:35.0
17:01:41.78 -29:42:14.3
17:15:16.25 -31:53:11.8
17:08:51.06 -31:31:17.8
17:15:40.42 -34:06:49.2
16:31:56.21 -29:30:24.0
17:07:45.51 -30:09:56.3
17:11:56.83 -34:42:53.1
17:08:14.69 -32:31:01.1
16:53:30.55 -30:17:16.3
16:08:28.73 -29:05:13.5
17:13:21.01 -34:28:01.4
16:58:21.05 -32:42:20.4
17:18:37.42 -33:33:16.6
17:17:40.16 -33:57:09.2
17:16:25.48 -31:00:17.7
16:29:23.88 -34:39:51.1
16:57:34.42 -35:29:47.1
17:14:11.24 -29:44:46.6
17:13:01.67 -29:45:35.0
17:02:12.15 -29:49:26.5
17:03:16.51 -36:59:28.9
16:56:42.22 -33:01:39.8
17:14:21.33 -36:25:37.2
17:18:42.13 -31:42:06.3
16:57:54.80 -34:01:26.8
16:54:22.78 -33:49:48.7
16:56:46.53 -31:53:30.7
16:56:02.72 -31:35:10.6
17:19:04.63 -35:33:37.2
17:10:32.33 -33:53:47.0
16:35:14.34 -32:36:04.2
17:11:05.92 -35:56:16.3
17:00:20.92 -32:19:27.7
17:02:11.74 -30:24:53.6
17:17:06.34 -30:27:55.2
17:18:42.63 -38:54:57.7
17:18:49.47 -33:16:46.0
16:55:02.23 -29:08:44.8
17:17:44.27 -31:55:06.2
16:34:16.70 -28:48:39.3
17:18:28.42 -31:54:27.5
17:07:12.75 -34:32:48.7
17:04:38.99 -32:54:51.3
16:57:53.48 -38:18:05.0
17:17:47.69 -35:29:43.8
17:02:44.01 -32:51:45.7
17:00:22.23 -37:58:54.5
16:18:19.40 -30:33:40.5
17:04:39.60 -29:29:29.5
17:12:25.88 -32:17:22.8
16:36:59.95 -32:19:26.1
16:27:35.92 -28:55:12.4
17:16:48.51 -32:59:45.2
16:16:43.33 -30:21:46.3
17:03:29.51 -38:55:02.4
16:57:46.01 -38:11:16.1
17:17:32.55 -38:53:41.1
16:32:31.12 -31:11:11.3
17:02:45.51 -38:37:42.6
17:14:36.32 -30:26:45.6
17:09:39.39 -30:57:10.5
17:17:47.50 -31:46:55.0
16:41:24.18 -37:16:56.1
16:59:55.55 -30:23:14.1
17:03:06.87 -29:12:46.4
17:12:29.17 -32:53:08.8
17:18:01.47 -30:51:50.3
16:25:27.34 -33:05:14.5
16:55:07.11 -32:17:24.7
16:49:47.77 -29:37:09.7
17:15:52.02 -30:21:28.2
17:08:09.86 -38:15:02.7
16:40:24.64 -33:52:43.8
16:38:36.61 -33:41:08.9
17:00:46.12 -29:56:37.8
16:56:57.63 -29:42:24.6
17:10:04.99 -29:34:54.0
17:14:24.17 -29:56:43.2
16:18:59.22 -28:42:47.3
16:21:23.92 -28:47:32.6
16:33:10.55 -33:11:25.5
16:13:21.16 -29:16:11.2
17:12:20.23 -32:31:20.9
17:16:00.93 -38:29:25.9
17:16:49.50 -33:23:00.6
17:03:20.42 -31:51:26.8
16:36:02.16 -29:53:13.6
16:59:41.35 -35:27:22.8
16:40:12.39 -33:23:43.9
16:34:42.00 -35:17:10.6
17:05:07.18 -32:51:51.1
16:39:17.97 -33:53:06.4
17:18:14.95 -31:59:33.6
17:00:08.21 -33:10:10.2
17:11:28.35 -34:05:16.7
16:18:01.24 -30:34:20.8
17:10:56.66 -29:29:35.0
16:25:27.91 -33:05:08.9
17:11:22.10 -30:30:59.8
17:16:24.49 -38:45:25.6
17:10:41.84 -35:57:57.6
17:17:47.81 -38:48:58.3
16:59:09.90 -33:57:53.5
16:58:28.79 -32:43:31.3
17:17:53.04 -31:07:14.2
16:32:00.77 -33:42:12.0
17:12:56.79 -33:27:03.8
17:12:06.50 -34:05:49.9
16:57:05.48 -32:36:13.4
16:33:41.90 -31:28:08.0
17:16:31.36 -38:56:29.8
16:53:07.13 -33:39:21.0
16:33:08.17 -31:51:28.6
17:04:44.10 -39:12:07.9
16:23:10.08 -33:32:47.7
17:13:56.09 -38:54:28.8
16:30:01.94 -32:44:22.1
17:00:33.97 -29:09:13.4
16:43:23.89 -31:49:42.9
16:30:08.80 -29:38:42.4
17:19:14.68 -38:39:06.4
16:55:25.41 -32:56:17.8
17:13:46.60 -31:34:10.3
17:10:04.15 -38:57:28.6
17:17:11.17 -38:59:26.4
16:29:29.22 -32:06:22.6
17:13:51.33 -38:55:08.4
17:14:16.41 -31:34:15.0
17:15:14.90 -39:04:50.3
17:15:29.57 -31:40:47.3
17:17:00.71 -38:51:45.9
16:12:39.76 -29:04:28.9
17:07:41.29 -38:22:47.5
17:17:18.97 -38:35:38.2
16:26:32.01 -33:51:01.9
16:45:55.67 -32:39:45.8
17:16:02.81 -38:54:46.3
16:12:14.88 -28:54:01.4
16:57:47.71 -38:32:22.1
17:15:35.56 -38:45:29.9
17:16:20.21 -39:07:24.3
16:23:54.97 -30:49:20.7
16:19:43.40 -30:08:09.0
16:12:15.31 -28:53:56.4
16:28:17.67 -28:54:10.6
16:46:15.71 -36:11:59.5
17:18:30.87 -39:07:58.9
17:07:33.26 -32:26:25.4
16:41:18.04 -34:07:33.8
17:11:35.39 -38:49:24.4
17:12:33.21 -35:28:44.8
16:40:12.62 -30:59:35.1
17:15:25.92 -38:59:36.5
16:47:07.43 -32:19:33.4
16:24:43.63 -33:41:27.1
17:04:48.86 -37:14:01.9
17:04:25.87 -37:06:41.0
17:11:52.06 -36:02:32.8
17:12:37.15 -35:57:26.4
16:34:17.40 -35:05:54.4
16:36:18.59 -34:36:04.9
17:00:08.83 -34:37:50.1
16:25:05.26 -33:45:19.2
17:16:52.77 -33:40:14.0
17:14:58.66 -33:14:36.7
16:54:47.09 -33:18:20.7
17:18:11.74 -32:59:05.9
16:39:13.71 -32:57:30.1
16:08:50.10 -28:36:08.5
16:53:11.20 -29:07:44.3
17:00:05.35 -29:13:32.6
16:10:17.33 -28:46:49.0
16:49:15.77 -29:29:41.6
16:16:07.16 -31:53:46.7
16:14:41.52 -32:23:33.3
17:15:43.32 -29:42:31.9
17:15:39.56 -30:04:49.2
17:06:08.68 -30:25:11.8
17:05:17.68 -30:31:15.0
17:12:00.02 -30:55:02.1
17:16:24.37 -31:00:15.1
17:13:47.97 -31:28:43.7
17:10:14.57 -31:33:19.1
17:15:22.44 -31:34:00.8
17:17:44.59 -32:12:06.2
17:02:43.50 -32:43:12.4
17:08:01.51 -32:57:09.6
16:16:21.69 -29:31:57.9
16:08:22.37 -29:54:32.7
17:01:12.37 -30:06:49.9
16:17:05.53 -29:41:47.6
16:17:07.79 -29:41:29.2
16:15:12.09 -29:43:21.2
16:08:29.08 -30:33:42.6
16:20:04.33 -31:00:57.0
16:20:21.52 -31:05:26.1
17:13:41.16 -31:53:02.3
16:56:56.92 -32:31:28.2
########### Completed Sco-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
17:17:36.70 -34:34:47.8
17:15:19.44 -30:12:23.3
17:13:54.15 -37:48:17.3
17:04:28.99 -37:57:06.4
17:16:25.34 -31:17:02.7
16:39:18.32 -31:53:30.8
16:41:47.25 -31:25:36.9
16:34:10.45 -34:51:10.4
17:18:31.45 -38:27:12.5
17:04:34.88 -37:58:21.5
17:01:31.06 -30:44:51.4
17:16:53.94 -29:54:49.4
17:18:18.07 -37:59:00.5
17:13:08.50 -29:18:02.7
17:19:01.25 -38:48:51.7
17:17:38.99 -29:47:13.0
17:18:16.05 -29:22:22.6
16:54:33.21 -38:05:47.5
17:17:58.57 -35:50:15.3
17:14:32.20 -29:27:46.9
16:53:57.62 -30:38:59.6
16:44:25.07 -33:02:04.4
16:47:58.53 -35:08:30.4
16:59:49.57 -29:47:38.7
16:33:45.56 -32:35:47.4
16:20:46.44 -31:42:18.1
17:05:03.88 -35:01:09.1
16:39:29.03 -33:32:16.3
16:12:09.96 -31:20:03.5
17:00:03.64 -31:40:43.1
16:07:04.88 -31:10:44.2
16:19:38.37 -29:52:27.4
16:47:05.39 -36:04:39.3
16:38:57.39 -35:00:56.5
16:40:48.19 -32:42:11.0
16:54:36.98 -37:51:38.5
16:20:36.11 -32:17:42.0
17:15:49.22 -37:46:54.1
16:12:06.42 -31:44:16.0
16:38:42.80 -33:29:45.7
16:35:30.41 -33:47:05.2
16:49:36.21 -32:19:57.9
16:58:46.90 -35:25:52.6
16:54:42.27 -36:22:48.4
16:34:32.89 -34:01:30.6
16:10:12.44 -30:03:36.5
16:10:45.51 -30:21:54.4
16:35:46.88 -33:26:32.1
16:17:39.57 -32:18:55.5
16:10:04.39 -30:32:37.6
16:40:30.89 -37:11:57.4
16:08:07.11 -31:08:58.3
16:59:13.36 -29:36:15.5
17:11:40.66 -38:29:39.7
16:08:29.59 -30:30:05.6
16:48:47.59 -32:02:01.1
17:15:45.45 -32:40:17.9
16:06:31.09 -31:23:36.4
17:15:20.12 -34:44:38.1
16:55:53.04 -39:13:40.1
16:11:44.57 -29:32:08.6
16:34:43.50 -32:48:05.2
17:08:54.67 -33:06:40.2
16:08:30.31 -29:02:24.1
16:59:42.24 -29:43:44.1
16:57:04.19 -34:39:15.2
17:15:23.05 -34:30:14.9
17:13:56.70 -37:45:16.7
16:06:52.62 -31:18:49.5
17:14:32.29 -36:34:46.3
17:09:49.50 -30:16:59.6
16:55:54.10 -30:55:44.7
16:33:42.10 -32:28:30.2
17:09:12.12 -33:51:25.4
16:50:02.95 -32:25:41.0
17:14:55.87 -35:14:25.0
17:16:14.77 -31:40:34.2
16:08:14.47 -29:27:57.8
17:17:10.54 -38:18:35.5
17:14:33.67 -35:05:17.6
17:12:56.78 -36:19:47.3
17:08:38.56 -33:39:27.0
17:15:38.51 -38:41:20.7
16:24:05.18 -33:09:32.6
17:14:27.90 -38:23:13.9
17:13:45.71 -38:30:58.8
17:13:46.55 -38:11:23.4
17:04:56.93 -34:09:55.3
17:09:52.40 -31:23:07.5
17:06:36.52 -36:58:36.7
17:02:15.87 -29:35:17.9
17:18:54.90 -38:39:24.4
16:56:31.68 -38:02:14.6
17:04:17.68 -34:51:07.1
17:10:19.27 -36:58:43.6
17:15:52.98 -37:10:16.8
17:19:07.80 -37:44:49.2
17:18:09.76 -33:51:24.2
17:17:02.77 -39:07:28.3
17:17:17.85 -35:24:23.0
17:07:11.94 -37:29:54.4
17:14:27.24 -33:13:58.9
17:07:53.35 -38:28:22.7
17:18:28.67 -38:24:30.7
17:17:41.49 -37:21:08.4
17:18:56.40 -38:14:59.8
17:10:09.81 -34:45:07.0
17:17:43.41 -32:12:12.8
17:19:18.80 -37:18:39.6
17:16:44.85 -38:11:47.7
17:01:49.03 -39:17:06.0
17:16:26.99 -38:48:55.9
17:09:17.84 -36:40:48.3
17:17:53.85 -38:07:50.4
17:12:57.22 -38:27:39.7
17:18:08.44 -37:18:00.6
16:43:44.06 -33:09:04.5
16:45:14.29 -32:37:55.9
17:17:36.12 -34:34:48.1
17:10:19.76 -37:19:27.9
17:13:07.44 -29:17:51.5
17:11:46.36 -30:46:04.1
17:13:48.77 -31:28:34.7
17:09:57.39 -36:16:15.1
17:07:35.62 -37:23:12.6
17:16:00.43 -34:15:54.8
17:16:15.58 -31:28:19.6
17:12:06.86 -29:19:15.8
17:19:18.11 -38:18:12.0
17:17:18.08 -30:12:57.7
16:55:34.87 -30:46:13.8
17:16:08.50 -29:55:33.4
17:02:52.61 -35:07:36.9
17:16:15.11 -31:28:16.0
17:02:16.54 -31:09:52.9
16:09:21.33 -28:30:17.9
16:54:46.25 -33:52:12.8
17:18:52.49 -33:30:26.5
17:12:34.34 -29:51:02.2
17:09:27.44 -29:14:58.1
16:09:37.84 -28:19:20.5
17:03:57.16 -33:45:19.1
17:03:42.73 -37:10:09.8
16:56:59.41 -32:28:58.4
17:17:16.33 -34:14:59.8
16:13:45.17 -28:23:26.2
17:03:18.94 -29:32:30.4
16:46:53.92 -30:07:53.5
17:18:53.14 -32:15:51.0
16:59:06.66 -34:11:40.0
17:15:59.66 -36:43:10.3
17:10:37.80 -37:18:10.3
17:04:28.57 -38:02:43.6
16:55:59.64 -31:08:59.9
16:36:22.76 -31:28:14.4
16:54:27.43 -29:47:25.8
16:53:13.32 -36:14:14.2
16:52:04.64 -29:46:23.3
16:36:58.07 -30:57:11.1
16:30:10.43 -33:17:05.9
16:58:21.71 -32:42:10.4
17:12:52.47 -31:41:59.7
16:26:52.24 -29:16:57.4
16:45:32.01 -31:25:44.1
16:54:50.85 -33:22:43.8
17:13:23.06 -30:49:08.2
16:56:10.63 -38:19:46.4
17:13:37.51 -35:50:38.1
17:12:20.35 -32:31:29.0
16:35:15.24 -34:32:33.9
17:15:51.73 -38:29:22.1
16:34:45.34 -30:00:58.4
16:23:12.82 -28:53:21.9
17:04:06.40 -29:17:08.9
17:05:28.63 -29:20:22.6
16:53:28.33 -30:40:09.6
17:19:02.93 -33:18:48.5
17:16:18.46 -34:07:00.4
17:00:22.06 -37:59:01.4
16:25:47.25 -32:37:57.6
16:08:29.10 -29:05:14.9
17:01:18.19 -38:33:35.0
17:01:41.78 -29:42:14.3
17:15:16.25 -31:53:11.8
17:08:51.06 -31:31:17.8
17:15:40.42 -34:06:49.2
16:31:56.21 -29:30:24.0
17:07:45.51 -30:09:56.3
17:11:56.83 -34:42:53.1
17:08:14.69 -32:31:01.1
16:53:30.55 -30:17:16.3
16:08:28.73 -29:05:13.5
17:13:21.01 -34:28:01.4
16:58:21.05 -32:42:20.4
17:18:37.42 -33:33:16.6
17:17:40.16 -33:57:09.2
17:16:25.48 -31:00:17.7
16:29:23.88 -34:39:51.1
16:57:34.42 -35:29:47.1
17:14:11.24 -29:44:46.6
17:13:01.67 -29:45:35.0
17:02:12.15 -29:49:26.5
17:03:16.51 -36:59:28.9
16:56:42.22 -33:01:39.8
17:14:21.33 -36:25:37.2
17:18:42.13 -31:42:06.3
16:57:54.80 -34:01:26.8
16:54:22.78 -33:49:48.7
16:56:46.53 -31:53:30.7
16:56:02.72 -31:35:10.6
17:19:04.63 -35:33:37.2
17:10:32.33 -33:53:47.0
16:35:14.34 -32:36:04.2
17:11:05.92 -35:56:16.3
17:00:20.92 -32:19:27.7
17:02:11.74 -30:24:53.6
17:17:06.34 -30:27:55.2
17:18:42.63 -38:54:57.7
17:18:49.47 -33:16:46.0
16:55:02.23 -29:08:44.8
17:17:44.27 -31:55:06.2
16:34:16.70 -28:48:39.3
17:18:28.42 -31:54:27.5
17:07:12.75 -34:32:48.7
17:04:38.99 -32:54:51.3
16:57:53.48 -38:18:05.0
17:17:47.69 -35:29:43.8
17:02:44.01 -32:51:45.7
17:00:22.23 -37:58:54.5
16:18:19.40 -30:33:40.5
17:04:39.60 -29:29:29.5
17:12:25.88 -32:17:22.8
16:36:59.95 -32:19:26.1
16:27:35.92 -28:55:12.4
17:16:48.51 -32:59:45.2
16:16:43.33 -30:21:46.3
17:03:29.51 -38:55:02.4
16:57:46.01 -38:11:16.1
17:17:32.55 -38:53:41.1
16:32:31.12 -31:11:11.3
17:02:45.51 -38:37:42.6
17:14:36.32 -30:26:45.6
17:09:39.39 -30:57:10.5
17:17:47.50 -31:46:55.0
16:41:24.18 -37:16:56.1
16:59:55.55 -30:23:14.1
17:03:06.87 -29:12:46.4
17:12:29.17 -32:53:08.8
17:18:01.47 -30:51:50.3
16:25:27.34 -33:05:14.5
16:55:07.11 -32:17:24.7
16:49:47.77 -29:37:09.7
17:15:52.02 -30:21:28.2
17:08:09.86 -38:15:02.7
16:40:24.64 -33:52:43.8
16:38:36.61 -33:41:08.9
17:00:46.12 -29:56:37.8
16:56:57.63 -29:42:24.6
17:10:04.99 -29:34:54.0
17:14:24.17 -29:56:43.2
16:18:59.22 -28:42:47.3
16:21:23.92 -28:47:32.6
16:33:10.55 -33:11:25.5
16:13:21.16 -29:16:11.2
17:12:20.23 -32:31:20.9
17:16:00.93 -38:29:25.9
17:16:49.50 -33:23:00.6
17:03:20.42 -31:51:26.8
16:36:02.16 -29:53:13.6
16:59:41.35 -35:27:22.8
16:40:12.39 -33:23:43.9
16:34:42.00 -35:17:10.6
17:05:07.18 -32:51:51.1
16:39:17.97 -33:53:06.4
17:18:14.95 -31:59:33.6
17:00:08.21 -33:10:10.2
17:11:28.35 -34:05:16.7
16:18:01.24 -30:34:20.8
17:10:56.66 -29:29:35.0
16:25:27.91 -33:05:08.9
17:11:22.10 -30:30:59.8
17:16:24.49 -38:45:25.6
17:10:41.84 -35:57:57.6
17:17:47.81 -38:48:58.3
16:59:09.90 -33:57:53.5
16:58:28.79 -32:43:31.3
17:17:53.04 -31:07:14.2
16:32:00.77 -33:42:12.0
17:12:56.79 -33:27:03.8
17:12:06.50 -34:05:49.9
16:57:05.48 -32:36:13.4
16:33:41.90 -31:28:08.0
17:16:31.36 -38:56:29.8
16:53:07.13 -33:39:21.0
16:33:08.17 -31:51:28.6
17:04:44.10 -39:12:07.9
16:23:10.08 -33:32:47.7
17:13:56.09 -38:54:28.8
16:30:01.94 -32:44:22.1
17:00:33.97 -29:09:13.4
16:43:23.89 -31:49:42.9
16:30:08.80 -29:38:42.4
17:19:14.68 -38:39:06.4
16:55:25.41 -32:56:17.8
17:13:46.60 -31:34:10.3
17:10:04.15 -38:57:28.6
17:17:11.17 -38:59:26.4
16:29:29.22 -32:06:22.6
17:13:51.33 -38:55:08.4
17:14:16.41 -31:34:15.0
17:15:14.90 -39:04:50.3
17:15:29.57 -31:40:47.3
17:17:00.71 -38:51:45.9
16:12:39.76 -29:04:28.9
17:07:41.29 -38:22:47.5
17:17:18.97 -38:35:38.2
16:26:32.01 -33:51:01.9
16:45:55.67 -32:39:45.8
17:16:02.81 -38:54:46.3
16:12:14.88 -28:54:01.4
16:57:47.71 -38:32:22.1
17:15:35.56 -38:45:29.9
17:16:20.21 -39:07:24.3
16:23:54.97 -30:49:20.7
16:19:43.40 -30:08:09.0
16:12:15.31 -28:53:56.4
16:28:17.67 -28:54:10.6
16:46:15.71 -36:11:59.5
17:18:30.87 -39:07:58.9
17:07:33.26 -32:26:25.4
16:41:18.04 -34:07:33.8
17:11:35.39 -38:49:24.4
17:12:33.21 -35:28:44.8
16:40:12.62 -30:59:35.1
17:15:25.92 -38:59:36.5
16:47:07.43 -32:19:33.4
16:24:43.63 -33:41:27.1
17:12:37.15 -35:57:26.4
16:17:07.79 -29:41:29.2
17:17:31.77 -38:57:25.7
16:17:05.53 -29:41:47.6
17:11:52.06 -36:02:32.8
16:54:47.09 -33:18:20.7
16:39:13.71 -32:57:30.1
16:52:04.56 -38:46:18.0
17:05:17.68 -30:31:15.0
17:16:24.37 -31:00:15.1
17:04:48.86 -37:14:01.9
16:53:11.20 -29:07:44.3
16:15:12.09 -29:43:21.2
17:08:01.51 -32:57:09.6
17:10:14.57 -31:33:19.1
17:17:11.38 -33:32:51.5
17:17:44.59 -32:12:06.2
17:02:43.50 -32:43:12.4
16:56:56.92 -32:31:28.2
16:49:15.77 -29:29:41.6
16:08:50.10 -28:36:08.5
16:20:04.33 -31:00:57.0
16:19:18.53 -32:29:03.2
16:16:21.69 -29:31:57.9
17:15:39.56 -30:04:49.2
16:16:07.16 -31:53:46.7
17:14:39.76 -34:28:15.9
17:15:43.32 -29:42:31.9
16:14:41.52 -32:23:33.3
17:00:08.83 -34:37:50.1
16:10:17.33 -28:46:49.0
17:00:05.35 -29:13:32.6
16:25:05.26 -33:45:19.2
16:08:22.37 -29:54:32.7
16:36:18.59 -34:36:04.9
16:34:17.40 -35:05:54.4
17:18:11.74 -32:59:05.9
17:06:08.68 -30:25:11.8
17:01:12.37 -30:06:49.9
17:15:22.44 -31:34:00.8
17:16:52.77 -33:40:14.0
17:04:25.87 -37:06:41.0
16:08:29.08 -30:33:42.6
17:13:47.97 -31:28:43.7
17:14:58.66 -33:14:36.7
17:13:41.16 -31:53:02.3
16:20:21.52 -31:05:26.1
17:12:00.02 -30:55:02.1
###################################################################################
17:17:36.70 -34:34:47.8 -- not an asteroid (will add it to exclusion list)
17:15:19.44 -30:12:23.3 -- not an asteroid (will add it to exclusion list)
17:13:54.15 -37:48:17.3 -- not an asteroid (will add it to exclusion list)
17:04:28.99 -37:57:06.4 -- not an asteroid (will add it to exclusion list)
17:16:25.34 -31:17:02.7 -- not an asteroid (will add it to exclusion list)
16:39:18.32 -31:53:30.8 -- not an asteroid (will add it to exclusion list)
16:41:47.25 -31:25:36.9 -- not an asteroid (will add it to exclusion list)
16:34:10.45 -34:51:10.4 -- not an asteroid (will add it to exclusion list)
17:18:31.45 -38:27:12.5 -- not an asteroid (will add it to exclusion list)
17:04:34.88 -37:58:21.5 -- not an asteroid (will add it to exclusion list)
17:01:31.06 -30:44:51.4 -- not an asteroid (will add it to exclusion list)
17:16:53.94 -29:54:49.4 -- not an asteroid (will add it to exclusion list)
17:18:18.07 -37:59:00.5 -- not an asteroid (will add it to exclusion list)
17:13:08.50 -29:18:02.7 -- not an asteroid (will add it to exclusion list)
17:19:01.25 -38:48:51.7 -- not an asteroid (will add it to exclusion list)
17:17:38.99 -29:47:13.0 -- not an asteroid (will add it to exclusion list)
17:18:16.05 -29:22:22.6 -- not an asteroid (will add it to exclusion list)
16:54:33.21 -38:05:47.5 -- not an asteroid (will add it to exclusion list)
17:17:58.57 -35:50:15.3 -- not an asteroid (will add it to exclusion list)
17:14:32.20 -29:27:46.9 -- not an asteroid (will add it to exclusion list)
16:53:57.62 -30:38:59.6 -- not an asteroid (will add it to exclusion list)
16:44:25.07 -33:02:04.4 -- not an asteroid (will add it to exclusion list)
16:47:58.53 -35:08:30.4 -- not an asteroid (will add it to exclusion list)
16:59:49.57 -29:47:38.7 -- not an asteroid (will add it to exclusion list)
16:33:45.56 -32:35:47.4 -- not an asteroid (will add it to exclusion list)
16:20:46.44 -31:42:18.1 -- not an asteroid (will add it to exclusion list)
17:05:03.88 -35:01:09.1 -- not an asteroid (will add it to exclusion list)
16:39:29.03 -33:32:16.3 -- not an asteroid (will add it to exclusion list)
16:12:09.96 -31:20:03.5 -- not an asteroid (will add it to exclusion list)
17:00:03.64 -31:40:43.1 -- not an asteroid (will add it to exclusion list)
16:07:04.88 -31:10:44.2 -- not an asteroid (will add it to exclusion list)
16:19:38.37 -29:52:27.4 -- not an asteroid (will add it to exclusion list)
16:47:05.39 -36:04:39.3 -- not an asteroid (will add it to exclusion list)
16:38:57.39 -35:00:56.5 -- asteroid (will NOT add it to exclusion list)
16:40:48.19 -32:42:11.0 -- not an asteroid (will add it to exclusion list)
16:54:36.98 -37:51:38.5 -- not an asteroid (will add it to exclusion list)
16:20:36.11 -32:17:42.0 -- not an asteroid (will add it to exclusion list)
17:15:49.22 -37:46:54.1 -- not an asteroid (will add it to exclusion list)
16:12:06.42 -31:44:16.0 -- not an asteroid (will add it to exclusion list)
16:38:42.80 -33:29:45.7 -- not an asteroid (will add it to exclusion list)
16:35:30.41 -33:47:05.2 -- not an asteroid (will add it to exclusion list)
16:49:36.21 -32:19:57.9 -- not an asteroid (will add it to exclusion list)
16:58:46.90 -35:25:52.6 -- not an asteroid (will add it to exclusion list)
16:54:42.27 -36:22:48.4 -- not an asteroid (will add it to exclusion list)
16:34:32.89 -34:01:30.6 -- not an asteroid (will add it to exclusion list)
16:10:12.44 -30:03:36.5 -- not an asteroid (will add it to exclusion list)
16:10:45.51 -30:21:54.4 -- not an asteroid (will add it to exclusion list)
16:35:46.88 -33:26:32.1 -- not an asteroid (will add it to exclusion list)
16:17:39.57 -32:18:55.5 -- not an asteroid (will add it to exclusion list)
16:10:04.39 -30:32:37.6 -- not an asteroid (will add it to exclusion list)
16:40:30.89 -37:11:57.4 -- not an asteroid (will add it to exclusion list)
16:08:07.11 -31:08:58.3 -- asteroid (will NOT add it to exclusion list)
16:59:13.36 -29:36:15.5 -- asteroid (will NOT add it to exclusion list)
17:11:40.66 -38:29:39.7 -- not an asteroid (will add it to exclusion list)
16:08:29.59 -30:30:05.6 -- not an asteroid (will add it to exclusion list)
16:48:47.59 -32:02:01.1 -- not an asteroid (will add it to exclusion list)
17:15:45.45 -32:40:17.9 -- not an asteroid (will add it to exclusion list)
16:06:31.09 -31:23:36.4 -- not an asteroid (will add it to exclusion list)
17:15:20.12 -34:44:38.1 -- not an asteroid (will add it to exclusion list)
16:55:53.04 -39:13:40.1 -- not an asteroid (will add it to exclusion list)
16:11:44.57 -29:32:08.6 -- not an asteroid (will add it to exclusion list)
16:34:43.50 -32:48:05.2 -- not an asteroid (will add it to exclusion list)
17:08:54.67 -33:06:40.2 -- not an asteroid (will add it to exclusion list)
16:08:30.31 -29:02:24.1 -- not an asteroid (will add it to exclusion list)
16:59:42.24 -29:43:44.1 -- not an asteroid (will add it to exclusion list)
16:57:04.19 -34:39:15.2 -- not an asteroid (will add it to exclusion list)
17:15:23.05 -34:30:14.9 -- not an asteroid (will add it to exclusion list)
17:13:56.70 -37:45:16.7 -- not an asteroid (will add it to exclusion list)
16:06:52.62 -31:18:49.5 -- not an asteroid (will add it to exclusion list)
17:14:32.29 -36:34:46.3 -- not an asteroid (will add it to exclusion list)
17:09:49.50 -30:16:59.6 -- not an asteroid (will add it to exclusion list)
16:55:54.10 -30:55:44.7 -- not an asteroid (will add it to exclusion list)
16:33:42.10 -32:28:30.2 -- not an asteroid (will add it to exclusion list)
17:09:12.12 -33:51:25.4 -- not an asteroid (will add it to exclusion list)
16:50:02.95 -32:25:41.0 -- not an asteroid (will add it to exclusion list)
17:14:55.87 -35:14:25.0 -- not an asteroid (will add it to exclusion list)
17:16:14.77 -31:40:34.2 -- not an asteroid (will add it to exclusion list)
16:08:14.47 -29:27:57.8 -- not an asteroid (will add it to exclusion list)
17:17:10.54 -38:18:35.5 -- not an asteroid (will add it to exclusion list)
17:14:33.67 -35:05:17.6 -- not an asteroid (will add it to exclusion list)
17:12:56.78 -36:19:47.3 -- not an asteroid (will add it to exclusion list)
17:08:38.56 -33:39:27.0 -- not an asteroid (will add it to exclusion list)
17:15:38.51 -38:41:20.7 -- not an asteroid (will add it to exclusion list)
16:24:05.18 -33:09:32.6 -- not an asteroid (will add it to exclusion list)
17:14:27.90 -38:23:13.9 -- not an asteroid (will add it to exclusion list)
17:13:45.71 -38:30:58.8 -- not an asteroid (will add it to exclusion list)
17:13:46.55 -38:11:23.4 -- not an asteroid (will add it to exclusion list)
17:04:56.93 -34:09:55.3 -- not an asteroid (will add it to exclusion list)
17:09:52.40 -31:23:07.5 -- not an asteroid (will add it to exclusion list)
17:06:36.52 -36:58:36.7 -- not an asteroid (will add it to exclusion list)
17:02:15.87 -29:35:17.9 -- not an asteroid (will add it to exclusion list)
17:18:54.90 -38:39:24.4 -- not an asteroid (will add it to exclusion list)
16:56:31.68 -38:02:14.6 -- not an asteroid (will add it to exclusion list)
17:04:17.68 -34:51:07.1 -- not an asteroid (will add it to exclusion list)
17:10:19.27 -36:58:43.6 -- not an asteroid (will add it to exclusion list)
17:15:52.98 -37:10:16.8 -- not an asteroid (will add it to exclusion list)
17:19:07.80 -37:44:49.2 -- not an asteroid (will add it to exclusion list)
17:18:09.76 -33:51:24.2 -- not an asteroid (will add it to exclusion list)
17:17:02.77 -39:07:28.3 -- not an asteroid (will add it to exclusion list)
17:17:17.85 -35:24:23.0 -- not an asteroid (will add it to exclusion list)
17:07:11.94 -37:29:54.4 -- not an asteroid (will add it to exclusion list)
17:14:27.24 -33:13:58.9 -- not an asteroid (will add it to exclusion list)
17:07:53.35 -38:28:22.7 -- not an asteroid (will add it to exclusion list)
17:18:28.67 -38:24:30.7 -- not an asteroid (will add it to exclusion list)
17:17:41.49 -37:21:08.4 -- not an asteroid (will add it to exclusion list)
17:18:56.40 -38:14:59.8 -- not an asteroid (will add it to exclusion list)
17:10:09.81 -34:45:07.0 -- not an asteroid (will add it to exclusion list)
17:17:43.41 -32:12:12.8 -- not an asteroid (will add it to exclusion list)
17:19:18.80 -37:18:39.6 -- not an asteroid (will add it to exclusion list)
17:16:44.85 -38:11:47.7 -- not an asteroid (will add it to exclusion list)
17:01:49.03 -39:17:06.0 -- not an asteroid (will add it to exclusion list)
17:16:26.99 -38:48:55.9 -- not an asteroid (will add it to exclusion list)
17:09:17.84 -36:40:48.3 -- not an asteroid (will add it to exclusion list)
17:17:53.85 -38:07:50.4 -- not an asteroid (will add it to exclusion list)
17:12:57.22 -38:27:39.7 -- not an asteroid (will add it to exclusion list)
17:18:08.44 -37:18:00.6 -- not an asteroid (will add it to exclusion list)
16:43:44.06 -33:09:04.5 -- not an asteroid (will add it to exclusion list)
16:45:14.29 -32:37:55.9 -- asteroid (will NOT add it to exclusion list)
17:17:36.12 -34:34:48.1 -- not an asteroid (will add it to exclusion list)
17:10:19.76 -37:19:27.9 -- not an asteroid (will add it to exclusion list)
17:13:07.44 -29:17:51.5 -- not an asteroid (will add it to exclusion list)
17:11:46.36 -30:46:04.1 -- not an asteroid (will add it to exclusion list)
17:13:48.77 -31:28:34.7 -- not an asteroid (will add it to exclusion list)
17:09:57.39 -36:16:15.1 -- not an asteroid (will add it to exclusion list)
17:07:35.62 -37:23:12.6 -- not an asteroid (will add it to exclusion list)
17:16:00.43 -34:15:54.8 -- not an asteroid (will add it to exclusion list)
17:16:15.58 -31:28:19.6 -- not an asteroid (will add it to exclusion list)
17:12:06.86 -29:19:15.8 -- not an asteroid (will add it to exclusion list)
17:19:18.11 -38:18:12.0 -- not an asteroid (will add it to exclusion list)
17:17:18.08 -30:12:57.7 -- not an asteroid (will add it to exclusion list)
16:55:34.87 -30:46:13.8 -- not an asteroid (will add it to exclusion list)
17:16:08.50 -29:55:33.4 -- not an asteroid (will add it to exclusion list)
17:02:52.61 -35:07:36.9 -- not an asteroid (will add it to exclusion list)
17:16:15.11 -31:28:16.0 -- not an asteroid (will add it to exclusion list)
17:02:16.54 -31:09:52.9 -- not an asteroid (will add it to exclusion list)
16:09:21.33 -28:30:17.9 -- not an asteroid (will add it to exclusion list)
16:54:46.25 -33:52:12.8 -- not an asteroid (will add it to exclusion list)
17:18:52.49 -33:30:26.5 -- not an asteroid (will add it to exclusion list)
17:12:34.34 -29:51:02.2 -- not an asteroid (will add it to exclusion list)
17:09:27.44 -29:14:58.1 -- not an asteroid (will add it to exclusion list)
16:09:37.84 -28:19:20.5 -- not an asteroid (will add it to exclusion list)
17:03:57.16 -33:45:19.1 -- not an asteroid (will add it to exclusion list)
17:03:42.73 -37:10:09.8 -- not an asteroid (will add it to exclusion list)
16:56:59.41 -32:28:58.4 -- asteroid (will NOT add it to exclusion list)
17:17:16.33 -34:14:59.8 -- not an asteroid (will add it to exclusion list)
16:13:45.17 -28:23:26.2 -- not an asteroid (will add it to exclusion list)
17:03:18.94 -29:32:30.4 -- not an asteroid (will add it to exclusion list)
16:46:53.92 -30:07:53.5 -- asteroid (will NOT add it to exclusion list)
17:18:53.14 -32:15:51.0 -- not an asteroid (will add it to exclusion list)
16:59:06.66 -34:11:40.0 -- not an asteroid (will add it to exclusion list)
17:15:59.66 -36:43:10.3 -- not an asteroid (will add it to exclusion list)
17:10:37.80 -37:18:10.3 -- not an asteroid (will add it to exclusion list)
17:04:28.57 -38:02:43.6 -- not an asteroid (will add it to exclusion list)
16:55:59.64 -31:08:59.9 -- not an asteroid (will add it to exclusion list)
16:36:22.76 -31:28:14.4 -- not an asteroid (will add it to exclusion list)
16:54:27.43 -29:47:25.8 -- not an asteroid (will add it to exclusion list)
16:53:13.32 -36:14:14.2 -- not an asteroid (will add it to exclusion list)
16:52:04.64 -29:46:23.3 -- not an asteroid (will add it to exclusion list)
16:36:58.07 -30:57:11.1 -- not an asteroid (will add it to exclusion list)
16:30:10.43 -33:17:05.9 -- not an asteroid (will add it to exclusion list)
16:58:21.71 -32:42:10.4 -- not an asteroid (will add it to exclusion list)
17:12:52.47 -31:41:59.7 -- not an asteroid (will add it to exclusion list)
16:26:52.24 -29:16:57.4 -- not an asteroid (will add it to exclusion list)
16:45:32.01 -31:25:44.1 -- not an asteroid (will add it to exclusion list)
16:54:50.85 -33:22:43.8 -- not an asteroid (will add it to exclusion list)
17:13:23.06 -30:49:08.2 -- not an asteroid (will add it to exclusion list)
16:56:10.63 -38:19:46.4 -- not an asteroid (will add it to exclusion list)
17:13:37.51 -35:50:38.1 -- not an asteroid (will add it to exclusion list)
17:12:20.35 -32:31:29.0 -- not an asteroid (will add it to exclusion list)
16:35:15.24 -34:32:33.9 -- not an asteroid (will add it to exclusion list)
17:15:51.73 -38:29:22.1 -- not an asteroid (will add it to exclusion list)
16:34:45.34 -30:00:58.4 -- not an asteroid (will add it to exclusion list)
16:23:12.82 -28:53:21.9 -- not an asteroid (will add it to exclusion list)
17:04:06.40 -29:17:08.9 -- not an asteroid (will add it to exclusion list)
17:05:28.63 -29:20:22.6 -- not an asteroid (will add it to exclusion list)
16:53:28.33 -30:40:09.6 -- not an asteroid (will add it to exclusion list)
17:19:02.93 -33:18:48.5 -- not an asteroid (will add it to exclusion list)
17:16:18.46 -34:07:00.4 -- not an asteroid (will add it to exclusion list)
17:00:22.06 -37:59:01.4 -- not an asteroid (will add it to exclusion list)
16:25:47.25 -32:37:57.6 -- not an asteroid (will add it to exclusion list)
16:08:29.10 -29:05:14.9 -- not an asteroid (will add it to exclusion list)
17:01:18.19 -38:33:35.0 -- not an asteroid (will add it to exclusion list)
17:01:41.78 -29:42:14.3 -- asteroid (will NOT add it to exclusion list)
17:15:16.25 -31:53:11.8 -- not an asteroid (will add it to exclusion list)
17:08:51.06 -31:31:17.8 -- not an asteroid (will add it to exclusion list)
17:15:40.42 -34:06:49.2 -- not an asteroid (will add it to exclusion list)
16:31:56.21 -29:30:24.0 -- not an asteroid (will add it to exclusion list)
17:07:45.51 -30:09:56.3 -- not an asteroid (will add it to exclusion list)
17:11:56.83 -34:42:53.1 -- not an asteroid (will add it to exclusion list)
17:08:14.69 -32:31:01.1 -- not an asteroid (will add it to exclusion list)
16:53:30.55 -30:17:16.3 -- not an asteroid (will add it to exclusion list)
16:08:28.73 -29:05:13.5 -- not an asteroid (will add it to exclusion list)
17:13:21.01 -34:28:01.4 -- not an asteroid (will add it to exclusion list)
16:58:21.05 -32:42:20.4 -- not an asteroid (will add it to exclusion list)
17:18:37.42 -33:33:16.6 -- not an asteroid (will add it to exclusion list)
17:17:40.16 -33:57:09.2 -- not an asteroid (will add it to exclusion list)
17:16:25.48 -31:00:17.7 -- not an asteroid (will add it to exclusion list)
16:29:23.88 -34:39:51.1 -- not an asteroid (will add it to exclusion list)
16:57:34.42 -35:29:47.1 -- not an asteroid (will add it to exclusion list)
17:14:11.24 -29:44:46.6 -- not an asteroid (will add it to exclusion list)
17:13:01.67 -29:45:35.0 -- not an asteroid (will add it to exclusion list)
17:02:12.15 -29:49:26.5 -- not an asteroid (will add it to exclusion list)
17:03:16.51 -36:59:28.9 -- not an asteroid (will add it to exclusion list)
16:56:42.22 -33:01:39.8 -- not an asteroid (will add it to exclusion list)
17:14:21.33 -36:25:37.2 -- not an asteroid (will add it to exclusion list)
17:18:42.13 -31:42:06.3 -- not an asteroid (will add it to exclusion list)
16:57:54.80 -34:01:26.8 -- not an asteroid (will add it to exclusion list)
16:54:22.78 -33:49:48.7 -- not an asteroid (will add it to exclusion list)
16:56:46.53 -31:53:30.7 -- not an asteroid (will add it to exclusion list)
16:56:02.72 -31:35:10.6 -- not an asteroid (will add it to exclusion list)
17:19:04.63 -35:33:37.2 -- not an asteroid (will add it to exclusion list)
17:10:32.33 -33:53:47.0 -- not an asteroid (will add it to exclusion list)
16:35:14.34 -32:36:04.2 -- not an asteroid (will add it to exclusion list)
17:11:05.92 -35:56:16.3 -- not an asteroid (will add it to exclusion list)
17:00:20.92 -32:19:27.7 -- not an asteroid (will add it to exclusion list)
17:02:11.74 -30:24:53.6 -- not an asteroid (will add it to exclusion list)
17:17:06.34 -30:27:55.2 -- not an asteroid (will add it to exclusion list)
17:18:42.63 -38:54:57.7 -- not an asteroid (will add it to exclusion list)
17:18:49.47 -33:16:46.0 -- not an asteroid (will add it to exclusion list)
16:55:02.23 -29:08:44.8 -- not an asteroid (will add it to exclusion list)
17:17:44.27 -31:55:06.2 -- not an asteroid (will add it to exclusion list)
16:34:16.70 -28:48:39.3 -- not an asteroid (will add it to exclusion list)
17:18:28.42 -31:54:27.5 -- not an asteroid (will add it to exclusion list)
17:07:12.75 -34:32:48.7 -- not an asteroid (will add it to exclusion list)
17:04:38.99 -32:54:51.3 -- not an asteroid (will add it to exclusion list)
16:57:53.48 -38:18:05.0 -- not an asteroid (will add it to exclusion list)
17:17:47.69 -35:29:43.8 -- not an asteroid (will add it to exclusion list)
17:02:44.01 -32:51:45.7 -- not an asteroid (will add it to exclusion list)
17:00:22.23 -37:58:54.5 -- not an asteroid (will add it to exclusion list)
16:18:19.40 -30:33:40.5 -- not an asteroid (will add it to exclusion list)
17:04:39.60 -29:29:29.5 -- not an asteroid (will add it to exclusion list)
17:12:25.88 -32:17:22.8 -- not an asteroid (will add it to exclusion list)
16:36:59.95 -32:19:26.1 -- not an asteroid (will add it to exclusion list)
16:27:35.92 -28:55:12.4 -- not an asteroid (will add it to exclusion list)
17:16:48.51 -32:59:45.2 -- not an asteroid (will add it to exclusion list)
16:16:43.33 -30:21:46.3 -- not an asteroid (will add it to exclusion list)
17:03:29.51 -38:55:02.4 -- not an asteroid (will add it to exclusion list)
16:57:46.01 -38:11:16.1 -- not an asteroid (will add it to exclusion list)
17:17:32.55 -38:53:41.1 -- not an asteroid (will add it to exclusion list)
16:32:31.12 -31:11:11.3 -- not an asteroid (will add it to exclusion list)
17:02:45.51 -38:37:42.6 -- not an asteroid (will add it to exclusion list)
17:14:36.32 -30:26:45.6 -- not an asteroid (will add it to exclusion list)
17:09:39.39 -30:57:10.5 -- not an asteroid (will add it to exclusion list)
17:17:47.50 -31:46:55.0 -- not an asteroid (will add it to exclusion list)
16:41:24.18 -37:16:56.1 -- not an asteroid (will add it to exclusion list)
16:59:55.55 -30:23:14.1 -- not an asteroid (will add it to exclusion list)
17:03:06.87 -29:12:46.4 -- not an asteroid (will add it to exclusion list)
17:12:29.17 -32:53:08.8 -- not an asteroid (will add it to exclusion list)
17:18:01.47 -30:51:50.3 -- not an asteroid (will add it to exclusion list)
16:25:27.34 -33:05:14.5 -- not an asteroid (will add it to exclusion list)
16:55:07.11 -32:17:24.7 -- not an asteroid (will add it to exclusion list)
16:49:47.77 -29:37:09.7 -- not an asteroid (will add it to exclusion list)
17:15:52.02 -30:21:28.2 -- not an asteroid (will add it to exclusion list)
17:08:09.86 -38:15:02.7 -- not an asteroid (will add it to exclusion list)
16:40:24.64 -33:52:43.8 -- not an asteroid (will add it to exclusion list)
16:38:36.61 -33:41:08.9 -- not an asteroid (will add it to exclusion list)
17:00:46.12 -29:56:37.8 -- not an asteroid (will add it to exclusion list)
16:56:57.63 -29:42:24.6 -- not an asteroid (will add it to exclusion list)
17:10:04.99 -29:34:54.0 -- not an asteroid (will add it to exclusion list)
17:14:24.17 -29:56:43.2 -- not an asteroid (will add it to exclusion list)
16:18:59.22 -28:42:47.3 -- not an asteroid (will add it to exclusion list)
16:21:23.92 -28:47:32.6 -- not an asteroid (will add it to exclusion list)
16:33:10.55 -33:11:25.5 -- not an asteroid (will add it to exclusion list)
16:13:21.16 -29:16:11.2 -- not an asteroid (will add it to exclusion list)
17:12:20.23 -32:31:20.9 -- not an asteroid (will add it to exclusion list)
17:16:00.93 -38:29:25.9 -- not an asteroid (will add it to exclusion list)
17:16:49.50 -33:23:00.6 -- not an asteroid (will add it to exclusion list)
17:03:20.42 -31:51:26.8 -- not an asteroid (will add it to exclusion list)
16:36:02.16 -29:53:13.6 -- not an asteroid (will add it to exclusion list)
16:59:41.35 -35:27:22.8 -- not an asteroid (will add it to exclusion list)
16:40:12.39 -33:23:43.9 -- not an asteroid (will add it to exclusion list)
16:34:42.00 -35:17:10.6 -- not an asteroid (will add it to exclusion list)
17:05:07.18 -32:51:51.1 -- not an asteroid (will add it to exclusion list)
16:39:17.97 -33:53:06.4 -- not an asteroid (will add it to exclusion list)
17:18:14.95 -31:59:33.6 -- not an asteroid (will add it to exclusion list)
17:00:08.21 -33:10:10.2 -- not an asteroid (will add it to exclusion list)
17:11:28.35 -34:05:16.7 -- not an asteroid (will add it to exclusion list)
16:18:01.24 -30:34:20.8 -- not an asteroid (will add it to exclusion list)
17:10:56.66 -29:29:35.0 -- not an asteroid (will add it to exclusion list)
16:25:27.91 -33:05:08.9 -- not an asteroid (will add it to exclusion list)
17:11:22.10 -30:30:59.8 -- not an asteroid (will add it to exclusion list)
17:16:24.49 -38:45:25.6 -- not an asteroid (will add it to exclusion list)
17:10:41.84 -35:57:57.6 -- not an asteroid (will add it to exclusion list)
17:17:47.81 -38:48:58.3 -- not an asteroid (will add it to exclusion list)
16:59:09.90 -33:57:53.5 -- not an asteroid (will add it to exclusion list)
16:58:28.79 -32:43:31.3 -- not an asteroid (will add it to exclusion list)
17:17:53.04 -31:07:14.2 -- not an asteroid (will add it to exclusion list)
16:32:00.77 -33:42:12.0 -- not an asteroid (will add it to exclusion list)
17:12:56.79 -33:27:03.8 -- not an asteroid (will add it to exclusion list)
17:12:06.50 -34:05:49.9 -- not an asteroid (will add it to exclusion list)
16:57:05.48 -32:36:13.4 -- not an asteroid (will add it to exclusion list)
16:33:41.90 -31:28:08.0 -- not an asteroid (will add it to exclusion list)
17:16:31.36 -38:56:29.8 -- not an asteroid (will add it to exclusion list)
16:53:07.13 -33:39:21.0 -- not an asteroid (will add it to exclusion list)
16:33:08.17 -31:51:28.6 -- not an asteroid (will add it to exclusion list)
17:04:44.10 -39:12:07.9 -- not an asteroid (will add it to exclusion list)
16:23:10.08 -33:32:47.7 -- not an asteroid (will add it to exclusion list)
17:13:56.09 -38:54:28.8 -- not an asteroid (will add it to exclusion list)
16:30:01.94 -32:44:22.1 -- not an asteroid (will add it to exclusion list)
17:00:33.97 -29:09:13.4 -- not an asteroid (will add it to exclusion list)
16:43:23.89 -31:49:42.9 -- not an asteroid (will add it to exclusion list)
16:30:08.80 -29:38:42.4 -- not an asteroid (will add it to exclusion list)
17:19:14.68 -38:39:06.4 -- not an asteroid (will add it to exclusion list)
16:55:25.41 -32:56:17.8 -- not an asteroid (will add it to exclusion list)
17:13:46.60 -31:34:10.3 -- not an asteroid (will add it to exclusion list)
17:10:04.15 -38:57:28.6 -- not an asteroid (will add it to exclusion list)
17:17:11.17 -38:59:26.4 -- not an asteroid (will add it to exclusion list)
16:29:29.22 -32:06:22.6 -- not an asteroid (will add it to exclusion list)
17:13:51.33 -38:55:08.4 -- not an asteroid (will add it to exclusion list)
17:14:16.41 -31:34:15.0 -- not an asteroid (will add it to exclusion list)
17:15:14.90 -39:04:50.3 -- not an asteroid (will add it to exclusion list)
17:15:29.57 -31:40:47.3 -- not an asteroid (will add it to exclusion list)
17:17:00.71 -38:51:45.9 -- not an asteroid (will add it to exclusion list)
16:12:39.76 -29:04:28.9 -- not an asteroid (will add it to exclusion list)
17:07:41.29 -38:22:47.5 -- not an asteroid (will add it to exclusion list)
17:17:18.97 -38:35:38.2 -- not an asteroid (will add it to exclusion list)
16:26:32.01 -33:51:01.9 -- not an asteroid (will add it to exclusion list)
16:45:55.67 -32:39:45.8 -- not an asteroid (will add it to exclusion list)
17:16:02.81 -38:54:46.3 -- not an asteroid (will add it to exclusion list)
16:12:14.88 -28:54:01.4 -- not an asteroid (will add it to exclusion list)
16:57:47.71 -38:32:22.1 -- not an asteroid (will add it to exclusion list)
17:15:35.56 -38:45:29.9 -- not an asteroid (will add it to exclusion list)
17:16:20.21 -39:07:24.3 -- not an asteroid (will add it to exclusion list)
16:23:54.97 -30:49:20.7 -- not an asteroid (will add it to exclusion list)
16:19:43.40 -30:08:09.0 -- not an asteroid (will add it to exclusion list)
16:12:15.31 -28:53:56.4 -- not an asteroid (will add it to exclusion list)
16:28:17.67 -28:54:10.6 -- not an asteroid (will add it to exclusion list)
16:46:15.71 -36:11:59.5 -- not an asteroid (will add it to exclusion list)
17:18:30.87 -39:07:58.9 -- not an asteroid (will add it to exclusion list)
17:07:33.26 -32:26:25.4 -- not an asteroid (will add it to exclusion list)
16:41:18.04 -34:07:33.8 -- not an asteroid (will add it to exclusion list)
17:11:35.39 -38:49:24.4 -- not an asteroid (will add it to exclusion list)
17:12:33.21 -35:28:44.8 -- not an asteroid (will add it to exclusion list)
16:40:12.62 -30:59:35.1 -- not an asteroid (will add it to exclusion list)
17:15:25.92 -38:59:36.5 -- not an asteroid (will add it to exclusion list)
16:47:07.43 -32:19:33.4 -- not an asteroid (will add it to exclusion list)
16:24:43.63 -33:41:27.1 -- not an asteroid (will add it to exclusion list)
17:12:37.15 -35:57:26.4 -- not an asteroid (will add it to exclusion list)
16:17:07.79 -29:41:29.2 -- not an asteroid (will add it to exclusion list)
17:17:31.77 -38:57:25.7 -- not an asteroid (will add it to exclusion list)
16:17:05.53 -29:41:47.6 -- not an asteroid (will add it to exclusion list)
17:11:52.06 -36:02:32.8 -- not an asteroid (will add it to exclusion list)
16:54:47.09 -33:18:20.7 -- not an asteroid (will add it to exclusion list)
16:39:13.71 -32:57:30.1 -- not an asteroid (will add it to exclusion list)
16:52:04.56 -38:46:18.0 -- not an asteroid (will add it to exclusion list)
17:05:17.68 -30:31:15.0 -- not an asteroid (will add it to exclusion list)
17:16:24.37 -31:00:15.1 -- not an asteroid (will add it to exclusion list)
17:04:48.86 -37:14:01.9 -- not an asteroid (will add it to exclusion list)
16:53:11.20 -29:07:44.3 -- not an asteroid (will add it to exclusion list)
16:15:12.09 -29:43:21.2 -- not an asteroid (will add it to exclusion list)
17:08:01.51 -32:57:09.6 -- not an asteroid (will add it to exclusion list)
17:10:14.57 -31:33:19.1 -- not an asteroid (will add it to exclusion list)
17:17:11.38 -33:32:51.5 -- not an asteroid (will add it to exclusion list)
17:17:44.59 -32:12:06.2 -- not an asteroid (will add it to exclusion list)
17:02:43.50 -32:43:12.4 -- not an asteroid (will add it to exclusion list)
16:56:56.92 -32:31:28.2 -- asteroid (will NOT add it to exclusion list)
16:49:15.77 -29:29:41.6 -- not an asteroid (will add it to exclusion list)
16:08:50.10 -28:36:08.5 -- not an asteroid (will add it to exclusion list)
16:20:04.33 -31:00:57.0 -- not an asteroid (will add it to exclusion list)
16:19:18.53 -32:29:03.2 -- not an asteroid (will add it to exclusion list)
16:16:21.69 -29:31:57.9 -- not an asteroid (will add it to exclusion list)
17:15:39.56 -30:04:49.2 -- not an asteroid (will add it to exclusion list)
16:16:07.16 -31:53:46.7 -- not an asteroid (will add it to exclusion list)
17:14:39.76 -34:28:15.9 -- not an asteroid (will add it to exclusion list)
17:15:43.32 -29:42:31.9 -- not an asteroid (will add it to exclusion list)
16:14:41.52 -32:23:33.3 -- not an asteroid (will add it to exclusion list)
17:00:08.83 -34:37:50.1 -- not an asteroid (will add it to exclusion list)
16:10:17.33 -28:46:49.0 -- not an asteroid (will add it to exclusion list)
17:00:05.35 -29:13:32.6 -- not an asteroid (will add it to exclusion list)
16:25:05.26 -33:45:19.2 -- not an asteroid (will add it to exclusion list)
16:08:22.37 -29:54:32.7 -- not an asteroid (will add it to exclusion list)
16:36:18.59 -34:36:04.9 -- not an asteroid (will add it to exclusion list)
16:34:17.40 -35:05:54.4 -- not an asteroid (will add it to exclusion list)
17:18:11.74 -32:59:05.9 -- not an asteroid (will add it to exclusion list)
17:06:08.68 -30:25:11.8 -- not an asteroid (will add it to exclusion list)
17:01:12.37 -30:06:49.9 -- not an asteroid (will add it to exclusion list)
17:15:22.44 -31:34:00.8 -- not an asteroid (will add it to exclusion list)
17:16:52.77 -33:40:14.0 -- not an asteroid (will add it to exclusion list)
17:04:25.87 -37:06:41.0 -- not an asteroid (will add it to exclusion list)
16:08:29.08 -30:33:42.6 -- not an asteroid (will add it to exclusion list)
17:13:47.97 -31:28:43.7 -- not an asteroid (will add it to exclusion list)
17:14:58.66 -33:14:36.7 -- not an asteroid (will add it to exclusion list)
17:13:41.16 -31:53:02.3 -- not an asteroid (will add it to exclusion list)
16:20:21.52 -31:05:26.1 -- not an asteroid (will add it to exclusion list)
17:12:00.02 -30:55:02.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:06:31.09 -31:23:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:06:52.62 -31:18:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:04.88 -31:10:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:14.47 -29:27:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:22.37 -29:54:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:28.73 -29:05:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:29.08 -30:33:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:29.10 -29:05:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:29.59 -30:30:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:30.31 -29:02:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:50.10 -28:36:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:21.33 -28:30:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:37.84 -28:19:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:04.39 -30:32:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:12.44 -30:03:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:17.33 -28:46:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:45.51 -30:21:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:11:44.57 -29:32:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:06.42 -31:44:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:09.96 -31:20:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:14.88 -28:54:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:15.31 -28:53:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:39.76 -29:04:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:13:21.16 -29:16:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:13:45.17 -28:23:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:14:41.52 -32:23:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:15:12.09 -29:43:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:07.16 -31:53:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:21.69 -29:31:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:43.33 -30:21:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:05.53 -29:41:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:07.79 -29:41:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:39.57 -32:18:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:18:01.24 -30:34:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:18:19.40 -30:33:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:18:59.22 -28:42:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:18.53 -32:29:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:38.37 -29:52:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:43.40 -30:08:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:04.33 -31:00:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:21.52 -31:05:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:36.11 -32:17:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:46.44 -31:42:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:23.92 -28:47:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:10.08 -33:32:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:12.82 -28:53:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:54.97 -30:49:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:05.18 -33:09:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:43.63 -33:41:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:05.26 -33:45:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:27.34 -33:05:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:27.91 -33:05:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:47.25 -32:37:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:32.01 -33:51:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:52.24 -29:16:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:35.92 -28:55:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:28:17.67 -28:54:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:23.88 -34:39:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:29.22 -32:06:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:30:01.94 -32:44:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:30:08.80 -29:38:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:30:10.43 -33:17:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:31:56.21 -29:30:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:00.77 -33:42:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:31.12 -31:11:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:08.17 -31:51:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:10.55 -33:11:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:41.90 -31:28:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:42.10 -32:28:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:45.56 -32:35:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:10.45 -34:51:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:16.70 -28:48:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:17.40 -35:05:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:32.89 -34:01:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:42.00 -35:17:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:43.50 -32:48:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:45.34 -30:00:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:14.34 -32:36:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:15.24 -34:32:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:30.41 -33:47:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:46.88 -33:26:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:02.16 -29:53:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:18.59 -34:36:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:22.76 -31:28:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:58.07 -30:57:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:59.95 -32:19:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:36.61 -33:41:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:42.80 -33:29:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:13.71 -32:57:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:17.97 -33:53:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:18.32 -31:53:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:29.03 -33:32:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:12.39 -33:23:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:12.62 -30:59:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:24.64 -33:52:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:30.89 -37:11:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:48.19 -32:42:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:18.04 -34:07:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:24.18 -37:16:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:47.25 -31:25:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:23.89 -31:49:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:44.06 -33:09:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:25.07 -33:02:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:32.01 -31:25:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:55.67 -32:39:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:15.71 -36:11:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:05.39 -36:04:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:07.43 -32:19:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:58.53 -35:08:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:47.59 -32:02:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:15.77 -29:29:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:36.21 -32:19:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:47.77 -29:37:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:02.95 -32:25:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:04.56 -38:46:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:04.64 -29:46:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:07.13 -33:39:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:11.20 -29:07:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:13.32 -36:14:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:28.33 -30:40:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:30.55 -30:17:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:57.62 -30:38:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:22.78 -33:49:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:27.43 -29:47:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:33.21 -38:05:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:36.98 -37:51:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:42.27 -36:22:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:46.25 -33:52:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:47.09 -33:18:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:54:50.85 -33:22:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:02.23 -29:08:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:07.11 -32:17:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:25.41 -32:56:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:34.87 -30:46:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:53.04 -39:13:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:54.10 -30:55:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:59.64 -31:08:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:02.72 -31:35:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:10.63 -38:19:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:31.68 -38:02:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:42.22 -33:01:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:46.53 -31:53:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:57.63 -29:42:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:04.19 -34:39:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:05.48 -32:36:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:34.42 -35:29:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:46.01 -38:11:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:47.71 -38:32:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:53.48 -38:18:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:54.80 -34:01:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:21.05 -32:42:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:21.71 -32:42:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:28.79 -32:43:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:46.90 -35:25:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:06.66 -34:11:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:09.90 -33:57:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:41.35 -35:27:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:42.24 -29:43:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:49.57 -29:47:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:55.55 -30:23:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:03.64 -31:40:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:05.35 -29:13:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:08.21 -33:10:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:08.83 -34:37:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:20.92 -32:19:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:22.06 -37:59:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:22.23 -37:58:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:33.97 -29:09:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:46.12 -29:56:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:12.37 -30:06:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:18.19 -38:33:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:31.06 -30:44:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:49.03 -39:17:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:11.74 -30:24:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:12.15 -29:49:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:15.87 -29:35:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:16.54 -31:09:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:43.50 -32:43:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:44.01 -32:51:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:45.51 -38:37:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:52.61 -35:07:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:06.87 -29:12:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:16.51 -36:59:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:18.94 -29:32:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:20.42 -31:51:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:29.51 -38:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:42.73 -37:10:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:57.16 -33:45:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:06.40 -29:17:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:17.68 -34:51:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:25.87 -37:06:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:28.57 -38:02:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:28.99 -37:57:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:34.88 -37:58:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:38.99 -32:54:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:39.60 -29:29:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:44.10 -39:12:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:48.86 -37:14:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:56.93 -34:09:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:03.88 -35:01:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:07.18 -32:51:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:17.68 -30:31:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:28.63 -29:20:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:08.68 -30:25:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:36.52 -36:58:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:11.94 -37:29:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:12.75 -34:32:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:33.26 -32:26:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:35.62 -37:23:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:41.29 -38:22:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:45.51 -30:09:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:53.35 -38:28:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:01.51 -32:57:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:09.86 -38:15:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:14.69 -32:31:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:38.56 -33:39:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:51.06 -31:31:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:54.67 -33:06:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:12.12 -33:51:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:17.84 -36:40:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:27.44 -29:14:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:39.39 -30:57:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:49.50 -30:16:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:52.40 -31:23:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:57.39 -36:16:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:04.15 -38:57:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:04.99 -29:34:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:09.81 -34:45:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:14.57 -31:33:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:19.27 -36:58:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:19.76 -37:19:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:32.33 -33:53:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:37.80 -37:18:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:41.84 -35:57:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:56.66 -29:29:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:05.92 -35:56:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:22.10 -30:30:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:28.35 -34:05:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:35.39 -38:49:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:40.66 -38:29:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:46.36 -30:46:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:52.06 -36:02:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:56.83 -34:42:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:00.02 -30:55:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:06.50 -34:05:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:06.86 -29:19:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:20.23 -32:31:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:20.35 -32:31:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:25.88 -32:17:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:29.17 -32:53:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:33.21 -35:28:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:34.34 -29:51:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:37.15 -35:57:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:52.47 -31:41:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:56.78 -36:19:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:56.79 -33:27:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:57.22 -38:27:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:01.67 -29:45:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:07.44 -29:17:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:08.50 -29:18:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:21.01 -34:28:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:23.06 -30:49:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:37.51 -35:50:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:41.16 -31:53:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:45.71 -38:30:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:46.55 -38:11:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:46.60 -31:34:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:47.97 -31:28:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:48.77 -31:28:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:51.33 -38:55:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:54.15 -37:48:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:56.09 -38:54:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:13:56.70 -37:45:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:11.24 -29:44:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:16.41 -31:34:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:21.33 -36:25:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:24.17 -29:56:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:27.24 -33:13:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:27.90 -38:23:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:32.20 -29:27:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:32.29 -36:34:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:33.67 -35:05:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:36.32 -30:26:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:39.76 -34:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:55.87 -35:14:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:14:58.66 -33:14:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:14.90 -39:04:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:16.25 -31:53:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:19.44 -30:12:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:20.12 -34:44:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:22.44 -31:34:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:23.05 -34:30:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:25.92 -38:59:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:29.57 -31:40:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:35.56 -38:45:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:38.51 -38:41:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:39.56 -30:04:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:40.42 -34:06:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:43.32 -29:42:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:45.45 -32:40:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:49.22 -37:46:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:51.73 -38:29:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:52.02 -30:21:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:52.98 -37:10:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:15:59.66 -36:43:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:00.43 -34:15:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:00.93 -38:29:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:02.81 -38:54:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:08.50 -29:55:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:14.77 -31:40:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:15.11 -31:28:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:15.58 -31:28:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:18.46 -34:07:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:20.21 -39:07:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:24.37 -31:00:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:24.49 -38:45:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:25.34 -31:17:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:25.48 -31:00:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:26.99 -38:48:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:31.36 -38:56:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:44.85 -38:11:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:48.51 -32:59:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:49.50 -33:23:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:52.77 -33:40:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:53.94 -29:54:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:00.71 -38:51:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:02.77 -39:07:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:06.34 -30:27:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:10.54 -38:18:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:11.17 -38:59:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:11.38 -33:32:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:16.33 -34:14:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:17.85 -35:24:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:18.08 -30:12:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:18.97 -38:35:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:31.77 -38:57:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:32.55 -38:53:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:36.12 -34:34:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:36.70 -34:34:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:38.99 -29:47:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:40.16 -33:57:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:41.49 -37:21:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:43.41 -32:12:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:44.27 -31:55:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:44.59 -32:12:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:47.50 -31:46:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:47.69 -35:29:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:47.81 -38:48:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:53.04 -31:07:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:53.85 -38:07:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:17:58.57 -35:50:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:01.47 -30:51:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:08.44 -37:18:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:09.76 -33:51:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:11.74 -32:59:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:14.95 -31:59:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:16.05 -29:22:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:18.07 -37:59:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:28.42 -31:54:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:28.67 -38:24:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:30.87 -39:07:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:31.45 -38:27:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:37.42 -33:33:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:42.13 -31:42:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:42.63 -38:54:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:49.47 -33:16:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:52.49 -33:30:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:53.14 -32:15:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:54.90 -38:39:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:56.40 -38:14:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:01.25 -38:48:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:02.93 -33:18:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:04.63 -35:33:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:07.80 -37:44:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:14.68 -38:39:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:18.11 -38:18:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:18.80 -37:18:39.6 -- 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)
16:06:31.09 -31:23:36.4 -- not a known variable star
16:06:52.62 -31:18:49.5 -- not a known variable star
16:07:04.88 -31:10:44.2 -- not a known variable star
16:08:14.47 -29:27:57.8 -- not a known variable star
16:08:22.37 -29:54:32.7 -- not a known variable star
16:08:28.73 -29:05:13.5 -- a known variable star
16:08:29.08 -30:33:42.6 -- not a known variable star
16:08:29.10 -29:05:14.9 -- a known variable star
16:08:29.59 -30:30:05.6 -- not a known variable star
16:08:30.31 -29:02:24.1 -- not a known variable star
16:08:50.10 -28:36:08.5 -- a known variable star
16:09:21.33 -28:30:17.9 -- not a known variable star
16:09:37.84 -28:19:20.5 -- not a known variable star
16:10:04.39 -30:32:37.6 -- not a known variable star
16:10:12.44 -30:03:36.5 -- not a known variable star
16:10:17.33 -28:46:49.0 -- not a known variable star
16:10:45.51 -30:21:54.4 -- not a known variable star
16:11:44.57 -29:32:08.6 -- not a known variable star
16:12:06.42 -31:44:16.0 -- not a known variable star
16:12:09.96 -31:20:03.5 -- not a known variable star
16:12:14.88 -28:54:01.4 -- not a known variable star
16:12:15.31 -28:53:56.4 -- not a known variable star
16:12:39.76 -29:04:28.9 -- a known variable star
16:13:21.16 -29:16:11.2 -- not a known variable star
16:13:45.17 -28:23:26.2 -- not a known variable star
16:14:41.52 -32:23:33.3 -- a known variable star
16:15:12.09 -29:43:21.2 -- not a known variable star
16:16:07.16 -31:53:46.7 -- not a known variable star
16:16:21.69 -29:31:57.9 -- not a known variable star
16:16:43.33 -30:21:46.3 -- a known variable star
16:17:05.53 -29:41:47.6 -- not a known variable star
16:17:07.79 -29:41:29.2 -- not a known variable star
16:17:39.57 -32:18:55.5 -- not a known variable star
16:18:01.24 -30:34:20.8 -- a known variable star
16:18:19.40 -30:33:40.5 -- not a known variable star
16:18:59.22 -28:42:47.3 -- not a known variable star
16:19:18.53 -32:29:03.2 -- not a known variable star
16:19:38.37 -29:52:27.4 -- not a known variable star
16:19:43.40 -30:08:09.0 -- a known variable star
16:20:04.33 -31:00:57.0 -- not a known variable star
16:20:21.52 -31:05:26.1 -- not a known variable star
16:20:36.11 -32:17:42.0 -- a known variable star
16:20:46.44 -31:42:18.1 -- not a known variable star
16:21:23.92 -28:47:32.6 -- a known variable star
16:23:10.08 -33:32:47.7 -- not a known variable star
16:23:12.82 -28:53:21.9 -- a known variable star
16:23:54.97 -30:49:20.7 -- not a known variable star
16:24:05.18 -33:09:32.6 -- a known variable star
16:24:43.63 -33:41:27.1 -- not a known variable star
16:25:05.26 -33:45:19.2 -- not a known variable star
16:25:27.34 -33:05:14.5 -- not a known variable star
16:25:27.91 -33:05:08.9 -- not a known variable star
16:25:47.25 -32:37:57.6 -- a known variable star
16:26:32.01 -33:51:01.9 -- a known variable star
16:26:52.24 -29:16:57.4 -- a known variable star
16:27:35.92 -28:55:12.4 -- not a known variable star
16:28:17.67 -28:54:10.6 -- not a known variable star
16:29:23.88 -34:39:51.1 -- not a known variable star
16:29:29.22 -32:06:22.6 -- not a known variable star
16:30:01.94 -32:44:22.1 -- not a known variable star
16:30:08.80 -29:38:42.4 -- not a known variable star
16:30:10.43 -33:17:05.9 -- not a known variable star
16:31:56.21 -29:30:24.0 -- not a known variable star
16:32:00.77 -33:42:12.0 -- not a known variable star
16:32:31.12 -31:11:11.3 -- not a known variable star
16:33:08.17 -31:51:28.6 -- not a known variable star
16:33:10.55 -33:11:25.5 -- not a known variable star
16:33:41.90 -31:28:08.0 -- not a known variable star
16:33:42.10 -32:28:30.2 -- not a known variable star
16:33:45.56 -32:35:47.4 -- not a known variable star
16:34:10.45 -34:51:10.4 -- not a known variable star
16:34:16.70 -28:48:39.3 -- not a known variable star
16:34:17.40 -35:05:54.4 -- a known variable star
16:34:32.89 -34:01:30.6 -- not a known variable star
16:34:42.00 -35:17:10.6 -- not a known variable star
16:34:43.50 -32:48:05.2 -- not a known variable star
16:34:45.34 -30:00:58.4 -- not a known variable star
16:35:14.34 -32:36:04.2 -- not a known variable star
16:35:15.24 -34:32:33.9 -- not a known variable star
16:35:30.41 -33:47:05.2 -- not a known variable star
16:35:46.88 -33:26:32.1 -- not a known variable star
16:36:02.16 -29:53:13.6 -- not a known variable star
16:36:18.59 -34:36:04.9 -- not a known variable star
16:36:22.76 -31:28:14.4 -- not a known variable star
16:36:58.07 -30:57:11.1 -- a known variable star
16:36:59.95 -32:19:26.1 -- not a known variable star
16:38:36.61 -33:41:08.9 -- not a known variable star
16:38:42.80 -33:29:45.7 -- not a known variable star
16:39:13.71 -32:57:30.1 -- a known variable star
16:39:17.97 -33:53:06.4 -- not a known variable star
16:39:18.32 -31:53:30.8 -- a known variable star
16:39:29.03 -33:32:16.3 -- not a known variable star
16:40:12.39 -33:23:43.9 -- not a known variable star
16:40:12.62 -30:59:35.1 -- not a known variable star
16:40:24.64 -33:52:43.8 -- not a known variable star
16:40:30.89 -37:11:57.4 -- not a known variable star
16:40:48.19 -32:42:11.0 -- a known variable star
16:41:18.04 -34:07:33.8 -- not a known variable star
16:41:24.18 -37:16:56.1 -- a known variable star
16:41:47.25 -31:25:36.9 -- not a known variable star
16:43:23.89 -31:49:42.9 -- not a known variable star
16:43:44.06 -33:09:04.5 -- not a known variable star
16:44:25.07 -33:02:04.4 -- not a known variable star
16:45:32.01 -31:25:44.1 -- not a known variable star
16:45:55.67 -32:39:45.8 -- a known variable star
16:46:15.71 -36:11:59.5 -- not a known variable star
16:47:05.39 -36:04:39.3 -- not a known variable star
16:47:07.43 -32:19:33.4 -- not a known variable star
16:47:58.53 -35:08:30.4 -- not a known variable star
16:48:47.59 -32:02:01.1 -- not a known variable star
16:49:15.77 -29:29:41.6 -- not a known variable star
16:49:36.21 -32:19:57.9 -- not a known variable star
16:49:47.77 -29:37:09.7 -- not a known variable star
16:50:02.95 -32:25:41.0 -- a known variable star
16:52:04.56 -38:46:18.0 -- not a known variable star
16:52:04.64 -29:46:23.3 -- not a known variable star
16:53:07.13 -33:39:21.0 -- a known variable star
16:53:11.20 -29:07:44.3 -- not a known variable star
16:53:13.32 -36:14:14.2 -- not a known variable star
16:53:28.33 -30:40:09.6 -- not a known variable star
16:53:30.55 -30:17:16.3 -- not a known variable star
16:53:57.62 -30:38:59.6 -- not a known variable star
16:54:22.78 -33:49:48.7 -- not a known variable star
16:54:27.43 -29:47:25.8 -- not a known variable star
16:54:33.21 -38:05:47.5 -- not a known variable star
16:54:36.98 -37:51:38.5 -- a known variable star
16:54:42.27 -36:22:48.4 -- a known variable star
16:54:46.25 -33:52:12.8 -- not a known variable star
16:54:47.09 -33:18:20.7 -- a known variable star
16:54:50.85 -33:22:43.8 -- not a known variable star
16:55:02.23 -29:08:44.8 -- not a known variable star
16:55:07.11 -32:17:24.7 -- not a known variable star
16:55:25.41 -32:56:17.8 -- a known variable star
16:55:34.87 -30:46:13.8 -- not a known variable star
16:55:53.04 -39:13:40.1 -- not a known variable star
16:55:54.10 -30:55:44.7 -- not a known variable star
16:55:59.64 -31:08:59.9 -- not a known variable star
16:56:02.72 -31:35:10.6 -- not a known variable star
16:56:10.63 -38:19:46.4 -- not a known variable star
16:56:31.68 -38:02:14.6 -- not a known variable star
16:56:42.22 -33:01:39.8 -- not a known variable star
16:56:46.53 -31:53:30.7 -- not a known variable star
16:56:57.63 -29:42:24.6 -- not a known variable star
16:57:04.19 -34:39:15.2 -- not a known variable star
16:57:05.48 -32:36:13.4 -- not a known variable star
16:57:34.42 -35:29:47.1 -- not a known variable star
16:57:46.01 -38:11:16.1 -- not a known variable star
16:57:47.71 -38:32:22.1 -- not a known variable star
16:57:53.48 -38:18:05.0 -- a known variable star
16:57:54.80 -34:01:26.8 -- not a known variable star
16:58:21.05 -32:42:20.4 -- not a known variable star
16:58:21.71 -32:42:10.4 -- not a known variable star
16:58:28.79 -32:43:31.3 -- a known variable star
16:58:46.90 -35:25:52.6 -- not a known variable star
16:59:06.66 -34:11:40.0 -- a known variable star
16:59:09.90 -33:57:53.5 -- not a known variable star
16:59:41.35 -35:27:22.8 -- not a known variable star
16:59:42.24 -29:43:44.1 -- a known variable star
16:59:49.57 -29:47:38.7 -- a known variable star
16:59:55.55 -30:23:14.1 -- a known variable star
17:00:03.64 -31:40:43.1 -- not a known variable star
17:00:05.35 -29:13:32.6 -- not a known variable star
17:00:08.21 -33:10:10.2 -- not a known variable star
17:00:08.83 -34:37:50.1 -- not a known variable star
17:00:20.92 -32:19:27.7 -- not a known variable star
17:00:22.06 -37:59:01.4 -- not a known variable star
17:00:22.23 -37:58:54.5 -- not a known variable star
17:00:33.97 -29:09:13.4 -- not a known variable star
17:00:46.12 -29:56:37.8 -- a known variable star
17:01:12.37 -30:06:49.9 -- a known variable star
17:01:18.19 -38:33:35.0 -- a known variable star
17:01:31.06 -30:44:51.4 -- not a known variable star
17:01:49.03 -39:17:06.0 -- a known variable star
17:02:11.74 -30:24:53.6 -- not a known variable star
17:02:12.15 -29:49:26.5 -- not a known variable star
17:02:15.87 -29:35:17.9 -- a known variable star
17:02:16.54 -31:09:52.9 -- not a known variable star
17:02:43.50 -32:43:12.4 -- not a known variable star
17:02:44.01 -32:51:45.7 -- a known variable star
17:02:45.51 -38:37:42.6 -- not a known variable star
17:02:52.61 -35:07:36.9 -- a known variable star
17:03:06.87 -29:12:46.4 -- a known variable star
17:03:16.51 -36:59:28.9 -- not a known variable star
17:03:18.94 -29:32:30.4 -- a known variable star
17:03:20.42 -31:51:26.8 -- not a known variable star
17:03:29.51 -38:55:02.4 -- not a known variable star
17:03:42.73 -37:10:09.8 -- a known variable star
17:03:57.16 -33:45:19.1 -- not a known variable star
17:04:06.40 -29:17:08.9 -- not a known variable star
17:04:17.68 -34:51:07.1 -- not a known variable star
17:04:25.87 -37:06:41.0 -- not a known variable star
17:04:28.57 -38:02:43.6 -- a known variable star
17:04:28.99 -37:57:06.4 -- a known variable star
17:04:34.88 -37:58:21.5 -- a known variable star
17:04:38.99 -32:54:51.3 -- not a known variable star
17:04:39.60 -29:29:29.5 -- not a known variable star
17:04:44.10 -39:12:07.9 -- not a known variable star
17:04:48.86 -37:14:01.9 -- not a known variable star
17:04:56.93 -34:09:55.3 -- not a known variable star
17:05:03.88 -35:01:09.1 -- a known variable star
17:05:07.18 -32:51:51.1 -- not a known variable star
17:05:17.68 -30:31:15.0 -- not a known variable star
17:05:28.63 -29:20:22.6 -- not a known variable star
17:06:08.68 -30:25:11.8 -- not a known variable star
17:06:36.52 -36:58:36.7 -- a known variable star
17:07:11.94 -37:29:54.4 -- a known variable star
17:07:12.75 -34:32:48.7 -- a known variable star
17:07:33.26 -32:26:25.4 -- not a known variable star
17:07:35.62 -37:23:12.6 -- not a known variable star
17:07:41.29 -38:22:47.5 -- a known variable star
17:07:45.51 -30:09:56.3 -- a known variable star
17:07:53.35 -38:28:22.7 -- a known variable star
17:08:01.51 -32:57:09.6 -- not a known variable star
17:08:09.86 -38:15:02.7 -- not a known variable star
17:08:14.69 -32:31:01.1 -- a known variable star
17:08:38.56 -33:39:27.0 -- not a known variable star
17:08:51.06 -31:31:17.8 -- a known variable star
17:08:54.67 -33:06:40.2 -- a known variable star
17:09:12.12 -33:51:25.4 -- a known variable star
17:09:17.84 -36:40:48.3 -- a known variable star
17:09:27.44 -29:14:58.1 -- not a known variable star
17:09:39.39 -30:57:10.5 -- not a known variable star
17:09:49.50 -30:16:59.6 -- a known variable star
17:09:52.40 -31:23:07.5 -- a known variable star
17:09:57.39 -36:16:15.1 -- not a known variable star
17:10:04.15 -38:57:28.6 -- not a known variable star
17:10:04.99 -29:34:54.0 -- a known variable star
17:10:09.81 -34:45:07.0 -- a known variable star
17:10:14.57 -31:33:19.1 -- not a known variable star
17:10:19.27 -36:58:43.6 -- not a known variable star
17:10:19.76 -37:19:27.9 -- a known variable star
17:10:32.33 -33:53:47.0 -- not a known variable star
17:10:37.80 -37:18:10.3 -- not a known variable star
17:10:41.84 -35:57:57.6 -- not a known variable star
17:10:56.66 -29:29:35.0 -- not a known variable star
17:11:05.92 -35:56:16.3 -- a known variable star
17:11:22.10 -30:30:59.8 -- not a known variable star
17:11:28.35 -34:05:16.7 -- not a known variable star
17:11:35.39 -38:49:24.4 -- not a known variable star
17:11:40.66 -38:29:39.7 -- not a known variable star
17:11:46.36 -30:46:04.1 -- not a known variable star
17:11:52.06 -36:02:32.8 -- a known variable star
17:11:56.83 -34:42:53.1 -- a known variable star
17:12:00.02 -30:55:02.1 -- not a known variable star
17:12:06.50 -34:05:49.9 -- a known variable star
17:12:06.86 -29:19:15.8 -- a known variable star
17:12:20.23 -32:31:20.9 -- not a known variable star
17:12:20.35 -32:31:29.0 -- not a known variable star
17:12:25.88 -32:17:22.8 -- a known variable star
17:12:29.17 -32:53:08.8 -- a known variable star
17:12:33.21 -35:28:44.8 -- a known variable star
17:12:34.34 -29:51:02.2 -- not a known variable star
17:12:37.15 -35:57:26.4 -- not a known variable star
17:12:52.47 -31:41:59.7 -- not a known variable star
17:12:56.78 -36:19:47.3 -- a known variable star
17:12:56.79 -33:27:03.8 -- not a known variable star
17:12:57.22 -38:27:39.7 -- not a known variable star
17:13:01.67 -29:45:35.0 -- a known variable star
17:13:07.44 -29:17:51.5 -- not a known variable star
17:13:08.50 -29:18:02.7 -- not a known variable star
17:13:21.01 -34:28:01.4 -- a known variable star
17:13:23.06 -30:49:08.2 -- not a known variable star
17:13:37.51 -35:50:38.1 -- not a known variable star
17:13:41.16 -31:53:02.3 -- a known variable star
17:13:45.71 -38:30:58.8 -- not a known variable star
17:13:46.55 -38:11:23.4 -- not a known variable star
17:13:46.60 -31:34:10.3 -- not a known variable star
17:13:47.97 -31:28:43.7 -- not a known variable star
17:13:48.77 -31:28:34.7 -- not a known variable star
17:13:51.33 -38:55:08.4 -- not a known variable star
17:13:54.15 -37:48:17.3 -- a known variable star
17:13:56.09 -38:54:28.8 -- a known variable star
17:13:56.70 -37:45:16.7 -- not a known variable star
17:14:11.24 -29:44:46.6 -- a known variable star
17:14:16.41 -31:34:15.0 -- not a known variable star
17:14:21.33 -36:25:37.2 -- not a known variable star
17:14:24.17 -29:56:43.2 -- not a known variable star
17:14:27.24 -33:13:58.9 -- not a known variable star
17:14:27.90 -38:23:13.9 -- not a known variable star
17:14:32.20 -29:27:46.9 -- a known variable star
17:14:32.29 -36:34:46.3 -- not a known variable star
17:14:33.67 -35:05:17.6 -- a known variable star
17:14:36.32 -30:26:45.6 -- not a known variable star
17:14:39.76 -34:28:15.9 -- not a known variable star
17:14:55.87 -35:14:25.0 -- a known variable star
17:14:58.66 -33:14:36.7 -- not a known variable star
17:15:14.90 -39:04:50.3 -- a known variable star
17:15:16.25 -31:53:11.8 -- a known variable star
17:15:19.44 -30:12:23.3 -- not a known variable star
17:15:20.12 -34:44:38.1 -- not a known variable star
17:15:22.44 -31:34:00.8 -- a known variable star
17:15:23.05 -34:30:14.9 -- not a known variable star
17:15:25.92 -38:59:36.5 -- not a known variable star
17:15:29.57 -31:40:47.3 -- not a known variable star
17:15:35.56 -38:45:29.9 -- not a known variable star
17:15:38.51 -38:41:20.7 -- not a known variable star
17:15:39.56 -30:04:49.2 -- not a known variable star
17:15:40.42 -34:06:49.2 -- not a known variable star
17:15:43.32 -29:42:31.9 -- a known variable star
17:15:45.45 -32:40:17.9 -- not a known variable star
17:15:49.22 -37:46:54.1 -- not a known variable star
17:15:51.73 -38:29:22.1 -- a known variable star
17:15:52.02 -30:21:28.2 -- a known variable star
17:15:52.98 -37:10:16.8 -- not a known variable star
17:15:59.66 -36:43:10.3 -- not a known variable star
17:16:00.43 -34:15:54.8 -- not a known variable star
17:16:00.93 -38:29:25.9 -- not a known variable star
17:16:02.81 -38:54:46.3 -- a known variable star
17:16:08.50 -29:55:33.4 -- a known variable star
17:16:14.77 -31:40:34.2 -- a known variable star
17:16:15.11 -31:28:16.0 -- a known variable star
17:16:15.58 -31:28:19.6 -- a known variable star
17:16:18.46 -34:07:00.4 -- a known variable star
17:16:20.21 -39:07:24.3 -- a known variable star
17:16:24.37 -31:00:15.1 -- a known variable star
17:16:24.49 -38:45:25.6 -- not a known variable star
17:16:25.34 -31:17:02.7 -- a known variable star
17:16:25.48 -31:00:17.7 -- a known variable star
17:16:26.99 -38:48:55.9 -- a known variable star
17:16:31.36 -38:56:29.8 -- a known variable star
17:16:44.85 -38:11:47.7 -- not a known variable star
17:16:48.51 -32:59:45.2 -- not a known variable star
17:16:49.50 -33:23:00.6 -- not a known variable star
17:16:52.77 -33:40:14.0 -- not a known variable star
17:16:53.94 -29:54:49.4 -- not a known variable star
17:17:00.71 -38:51:45.9 -- not a known variable star
17:17:02.77 -39:07:28.3 -- not a known variable star
17:17:06.34 -30:27:55.2 -- a known variable star
17:17:10.54 -38:18:35.5 -- a known variable star
17:17:11.17 -38:59:26.4 -- a known variable star
17:17:11.38 -33:32:51.5 -- not a known variable star
17:17:16.33 -34:14:59.8 -- not a known variable star
17:17:17.85 -35:24:23.0 -- a known variable star
17:17:18.08 -30:12:57.7 -- not a known variable star
17:17:18.97 -38:35:38.2 -- not a known variable star
17:17:31.77 -38:57:25.7 -- a known variable star
17:17:32.55 -38:53:41.1 -- not a known variable star
17:17:36.12 -34:34:48.1 -- not a known variable star
17:17:36.70 -34:34:47.8 -- not a known variable star
17:17:38.99 -29:47:13.0 -- not a known variable star
17:17:40.16 -33:57:09.2 -- a known variable star
17:17:41.49 -37:21:08.4 -- not a known variable star
17:17:43.41 -32:12:12.8 -- a known variable star
17:17:44.27 -31:55:06.2 -- not a known variable star
17:17:44.59 -32:12:06.2 -- a known variable star
17:17:47.50 -31:46:55.0 -- a known variable star
17:17:47.69 -35:29:43.8 -- not a known variable star
17:17:47.81 -38:48:58.3 -- a known variable star
17:17:53.04 -31:07:14.2 -- a known variable star
17:17:53.85 -38:07:50.4 -- not a known variable star
17:17:58.57 -35:50:15.3 -- not a known variable star
17:18:01.47 -30:51:50.3 -- not a known variable star
17:18:08.44 -37:18:00.6 -- not a known variable star
17:18:09.76 -33:51:24.2 -- not a known variable star
17:18:11.74 -32:59:05.9 -- a known variable star
17:18:14.95 -31:59:33.6 -- not a known variable star
17:18:16.05 -29:22:22.6 -- a known variable star
17:18:18.07 -37:59:00.5 -- not a known variable star
17:18:28.42 -31:54:27.5 -- not a known variable star
17:18:28.67 -38:24:30.7 -- not a known variable star
17:18:30.87 -39:07:58.9 -- a known variable star
17:18:31.45 -38:27:12.5 -- not a known variable star
17:18:37.42 -33:33:16.6 -- a known variable star
17:18:42.13 -31:42:06.3 -- not a known variable star
17:18:42.63 -38:54:57.7 -- not a known variable star
17:18:49.47 -33:16:46.0 -- not a known variable star
17:18:52.49 -33:30:26.5 -- a known variable star
17:18:53.14 -32:15:51.0 -- not a known variable star
17:18:54.90 -38:39:24.4 -- not a known variable star
17:18:56.40 -38:14:59.8 -- not a known variable star
17:19:01.25 -38:48:51.7 -- not a known variable star
17:19:02.93 -33:18:48.5 -- not a known variable star
17:19:04.63 -35:33:37.2 -- not a known variable star
17:19:07.80 -37:44:49.2 -- not a known variable star
17:19:14.68 -38:39:06.4 -- not a known variable star
17:19:18.11 -38:18:12.0 -- not a known variable star
17:19:18.80 -37:18:39.6 -- not a known variable star
Found 261 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
377 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 377 (excluding asteroids and hot pixels, 261 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461150.92753051 -observatory V36
00:31:37.73 +00:34:04.4 Mercury (-0.1mag)
03:30:29.02 +19:26:19.4 Venus (-3.9mag)
00:30:24.50 +02:14:36.1 Mars (1.2mag)
07:14:44.72 +22:42:40.9 Jupiter (-2.1mag)
00:31:08.41 +01:01:08.4 Saturn (0.9mag)
03:48:38.78 +19:50:30.0 Uranus (5.8mag)
00:11:24.71 -00:11:47.0 Neptune (7.8mag)
20:33:55.76 -22:52:52.5 Pluto (14.5mag)
04:34:11.04 +26:14:23.3 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 362 Apr 20 05:22 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461150.92753051:
07:14:46.97 +22:42:33.6 Io (5.8mag)
07:14:57.19 +22:42:13.2 Europa (5.9mag)
07:14:38.01 +22:43:01.8 Ganymede (5.4mag)
07:14:44.54 +22:42:31.8 Callisto (6.6mag)
07:17:52.73 +22:28:19.9 Himalia (15.4mag)
07:14:44.51 +22:42:43.6 Thebe (16.3mag)
07:18:09.44 +22:58:40.0 Elara (17.3mag)
07:13:55.68 +23:20:22.3 Pasiphae (17.4mag)
07:22:58.31 +22:41:06.8 Carme (18.5mag)
00:30:59.09 +01:01:21.4 Titan (8.8mag)
00:31:05.88 +01:01:14.7 Rhea (10.1mag)
00:30:42.15 +01:00:35.4 Iapetus (11.5mag)
00:31:00.38 +01:01:33.8 Hyperion (14.8mag)
00:32:41.68 +01:09:27.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 20 05:22 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461150.92753051:
15:55:30.35 -19:13:47.7 JWST
18:31:54.84 +26:59:22.1 Chandra
09:03:50.02 -51:39:01.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 20 05:22 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461150.92753051 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:35.57 -29:02:49.5 13.9mag P/2010 H2 (Vales)
05:10:00.15 -69:27:29.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:27.49 +31:28:07.5 17.2mag C/2017 K2 (PANSTARRS)
17:29:53.70 +11:03:57.4 17.6mag C/2021 G2 (ATLAS)
23:11:19.81 +29:24:36.8 17.1mag C/2022 E2 (ATLAS)
04:34:26.28 +26:09:20.6 16.1mag C/2022 N2 (PANSTARRS)
09:04:30.14 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:31:51.28 +00:18:15.3 17.4mag C/2022 R6 (PANSTARRS)
18:52:33.92 +18:53:54.8 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:09.88 -11:27:22.8 17.5mag P/2023 B1 (PANSTARRS)
09:05:44.76 -11:11:19.1 17.7mag C/2023 F3 (ATLAS)
21:58:25.99 +63:10:29.4 17.5mag C/2023 H5 (Lemmon)
19:15:02.16 -03:49:00.5 14.1mag C/2023 R1 (PANSTARRS)
21:20:00.29 +86:31:59.9 17.8mag C/2023 X2 (Lemmon)
06:20:14.10 +63:30:01.8 17.2mag C/2024 A1 (ATLAS)
05:22:32.65 +19:40:59.0 11.3mag C/2024 E1 (Wierzchos)
16:16:19.09 +07:06:42.6 17.3mag C/2024 G6 (ATLAS)
20:21:54.70 +16:29:40.0 14.5mag C/2024 J3 (ATLAS)
03:30:23.58 -21:43:24.9 16.3mag C/2024 T5 (ATLAS)
05:20:32.17 +44:13:01.6 17.7mag C/2025 J1 (Borisov)
13:20:41.14 +48:00:19.1 15.4mag C/2025 L1 (ATLAS)
03:32:25.81 -26:55:20.0 17.9mag C/2025 Q3 (ATLAS)
00:36:05.20 +16:01:33.9 8.0mag C/2025 R3 (PANSTARRS)
12:52:13.37 +03:16:24.2 17.4mag C/2025 Y1 (ATLAS)
03:59:40.32 +02:14:24.2 14.5mag C/2026 A1 (MAPS)
00:11:54.03 +37:59:46.3 14.7mag C/2026 B2 (Sun-Gao)
18:51:32.04 -09:28:43.3 11.6mag 10P/Tempel
14:54:14.93 +02:43:04.8 14.4mag 24P/Schaumasse
11:01:42.85 -01:23:25.2 15.7mag 29P/Schwassmann-Wachmann
10:37:36.77 -03:46:04.9 17.0mag 43P/Wolf-Harrington
01:55:32.71 +18:14:10.2 17.3mag 47P/Ashbrook-Jackson
07:19:05.30 +36:02:55.6 17.0mag 63P/Wild
23:34:38.36 -10:55:37.3 15.7mag 65P/Gunn
04:15:15.10 +22:44:07.3 15.9mag 76P/West-Kohoutek-Ikemura
01:15:25.21 +09:05:33.2 14.3mag 78P/Gehrels
23:16:13.22 -08:04:52.9 14.7mag 88P/Howell
02:23:04.49 +21:47:50.8 15.1mag 93P/Lovas
05:03:18.45 +32:30:43.1 16.1mag 123P/West-Hartley
08:33:49.18 +36:19:15.3 16.2mag 124P/Mrkos
02:40:06.14 +14:51:27.5 16.4mag 128P/Shoemaker-Holt
02:56:15.24 +15:01:13.8 17.5mag 131P/Mueller
01:49:41.86 +14:41:15.6 10.5mag 141P/Machholz
01:57:55.89 +06:31:15.1 10.5mag 141P-A/Machholz
00:41:17.59 +02:18:19.7 12.3mag 141P-D/Machholz
02:28:30.76 +08:16:13.2 17.9mag 141P-I/Machholz
01:14:46.77 +00:42:31.2 15.0mag 162P/SidingSpring
14:43:36.91 +00:21:07.7 17.8mag 210P/Christensen
21:51:16.30 -10:23:24.1 17.7mag 218P/LINEAR
17:17:17.34 -13:23:40.2 16.1mag 235P/LINEAR
05:44:08.02 +35:00:26.8 16.8mag 240P/NEAT
07:40:48.05 -04:42:14.5 17.8mag 242P/Spahr
22:27:59.44 -19:46:05.7 17.8mag 260P/McNaught
02:07:20.34 +21:34:03.2 18.0mag 295P/LINEAR
15:40:47.87 +07:16:12.9 17.5mag 391P/Kowalski
07:36:01.12 +21:22:23.3 17.7mag 450P/LONEOS
05:42:25.04 +44:46:25.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 20 05:22 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 20 05:22 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 20 05:22 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:24:19.761 -36:04:17.66 AT 2026jke 2026-04-06.51 19.98
11:16:25.694 -50:15:29.19 AT 2026jkd 2026-03-28.49 19.6
11:43:56.670 -49:03:17.42 AT 2026jkc 2026-04-12.46 19.35
11:38:21.891 -50:43:06.73 SN 2026jkb 2026-04-12.46 18.57
08:19:14.303 -28:43:36.53 AT 2026jka 2026-04-11.37 19.87
07:49:32.473 -24:44:26.65 AT 2026jjz 2026-04-12.39 18.98
14:44:18.498 -44:01:13.70 AT 2026jjy 2026-04-09.61 19.64
08:53:40.997 -38:26:31.85 AT 2026jjx 2026-03-23.40 20
12:26:02.763 -33:38:07.00 AT 2026jjw 2026-04-09.56 20.25
11:26:18.195 +19:38:31.94 AT 2026jjv 2026-04-06.91 19.81
11:33:29.132 -27:21:16.23 AT 2026jju 2026-04-12.45 19.32
12:15:03.964 -49:33:10.66 AT 2026jjt 2026-04-12.17 19.263
17:17:54.158 -75:07:32.46 AT 2026jjs 2026-04-12.30 19.194
08:35:23.434 +10:31:04.49 AT 2026jjr 2026-04-11.93 19.882
09:53:48.141 +08:12:51.52 AT 2026jjq 2026-04-11.92 20.219
12:47:33.422 +00:05:56.15 AT 2026jjp 2026-04-12.03 20.061
16:10:20.836 -68:49:59.48 AT 2026jjo 2026-04-12.26 19.161
18:36:22.563 -76:59:23.30 AT 2026jjn 2026-04-12.30 18.78
18:56:03.327 -40:52:01.58 AT 2026jjm 2026-04-12.35 18.51
16:42:43.663 -75:30:11.13 AT 2026jjl 2026-04-12.27 19.255
-rw-r--r-- 1 apache apache 30K Apr 20 05:22 tns_transients_list.txt
