This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6
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 6033015873537188352,2461150.9247,10.32,0.05,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
Gaia DR3 6033015873537188352 20260420.4247 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
ATO J253.3262-29.5226,2461150.9247,10.26,0.05,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
ATO J253.3262-29.5226 20260420.4247 10.26CV 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 6032914203067481984,2461150.9247,10.15,0.05,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 6032914203067481984 20260420.4247 10.15CV 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
ATO J250.7899-21.6891,2461150.9247,10.04,0.05,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
ATO J250.7899-21.6891 20260420.4247 10.04CV 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 6046236740616715520,2461150.9247,9.62,0.05,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 6046236740616715520 20260420.4247 9.62CV 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 6037645126698020224,2461150.9247,9.81,0.05,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 6037645126698020224 20260420.4247 9.81CV 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 6031416187195473024,2461150.9247,9.91,0.05,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 6031416187195473024 20260420.4247 9.91CV 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 6046552781485318912,2461150.9247,10.03,0.05,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 6046552781485318912 20260420.4247 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
ATO J243.3496-21.9511,2461150.9247,10.13,0.05,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
ATO J243.3496-21.9511 20260420.4247 10.13CV 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 4125383505927935232,2461150.9247,10.11,0.05,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 4125383505927935232 20260420.4247 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 6032976600345279872,2461150.9247,10.21,0.05,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 6032976600345279872 20260420.4247 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
VARIABLE_NAME,2461150.9247,10.24,0.05,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
VARIABLE_NAME 20260420.4247 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
VARIABLE_NAME,2461150.9247,10.25,0.05,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
VARIABLE_NAME 20260420.4247 10.25CV 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
VARIABLE_NAME,2461150.9247,10.36,0.05,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
VARIABLE_NAME 20260420.4247 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 6030788400382912384,2461150.9247,10.46,0.05,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 6030788400382912384 20260420.4247 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 6045465815462093696,2461150.9247,8.88,0.05,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 6045465815462093696 20260420.4247 8.88CV 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 6042185177704887936,2461150.9247,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6042185177704887936 20260420.4247 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6043706493779619456,2461150.9247,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6043706493779619456 20260420.4247 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J160818.96-271706.2,2461150.9247,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J160818.96-271706.2 20260420.4247 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J235.9186-28.4005,2461150.9247,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J235.9186-28.4005 20260420.4247 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233079087980888064,2461150.9247,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6233079087980888064 20260420.4247 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J235.8249-28.2823,2461150.9247,12.25,0.05,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
ATO J235.8249-28.2823 20260420.4247 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233464088851427328,2461150.9247,12.05,0.05,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 6233464088851427328 20260420.4247 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 6031175114962939008,2461150.9247,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6031175114962939008 20260420.4247 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9247,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4247 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6235600306805005056,2461150.9247,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6235600306805005056 20260420.4247 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.6946-29.4601,2461150.9247,12.15,0.05,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
ATO J236.6946-29.4601 20260420.4247 12.15CV 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
ASASSN-V J155951.15-280848.4,2461150.9247,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J155951.15-280848.4 20260420.4247 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.8901-28.3223,2461150.9247,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J237.8901-28.3223 20260420.4247 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J247.5982-30.0868,2461150.9247,12.00,0.05,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
ATO J247.5982-30.0868 20260420.4247 12.00CV 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 6240486158520609408,2461150.9247,11.52,0.05,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 6240486158520609408 20260420.4247 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J236.7124-28.3666,2461150.9247,11.95,0.05,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
ATO J236.7124-28.3666 20260420.4247 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
Gaia DR3 6233923448492583040,2461150.9247,11.89,0.05,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 6233923448492583040 20260420.4247 11.89CV 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 J162220.03-305121.6,2461150.9247,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J162220.03-305121.6 20260420.4247 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
Gaia DR3 6041733110927467776,2461150.9247,11.95,0.05,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 6041733110927467776 20260420.4247 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
Gaia DR3 6239749107770208256,2461150.9247,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6239749107770208256 20260420.4247 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J240.8377-28.7567,2461150.9247,11.94,0.05,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
ATO J240.8377-28.7567 20260420.4247 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 6240790822019689088,2461150.9247,11.41,0.05,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 6240790822019689088 20260420.4247 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 6041185657215817984,2461150.9247,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6041185657215817984 20260420.4247 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J155907-2150.7,2461150.9247,11.53,0.05,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
ASAS J155907-2150.7 20260420.4247 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 6236024409061930240,2461150.9247,11.62,0.05,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
Gaia DR3 6236024409061930240 20260420.4247 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
ASASSN-V J155008.16-233320.8,2461150.9247,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J155008.16-233320.8 20260420.4247 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 203252923,2461150.9247,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203252923 20260420.4247 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.7320-26.5847,2461150.9247,11.61,0.05,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
ATO J238.7320-26.5847 20260420.4247 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
Gaia DR3 6233224433975744768,2461150.9247,11.76,0.05,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 6233224433975744768 20260420.4247 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
ATO J237.8901-28.3223,2461150.9247,11.86,0.05,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
ATO J237.8901-28.3223 20260420.4247 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
ASAS J154437-2740.2,2461150.9247,11.63,0.05,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
ASAS J154437-2740.2 20260420.4247 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 6234834389575138048,2461150.9247,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6234834389575138048 20260420.4247 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 11.84 16:09:46.74 -30:23:54.2
345.88752 15.48230 galactic Sco Second-epoch detections are separated by 6.6" and 6.3 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 6038501337019179776 | 16:09:45.53 -30:24:04.6 (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 6038501337019179776,2461150.9247,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6038501337019179776 20260420.4247 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030848529950659200,2461150.9247,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030848529950659200 20260420.4247 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030760706453607168,2461150.9247,11.64,0.05,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 6030760706453607168 20260420.4247 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
ATO J238.7552-29.9681,2461150.9247,11.73,0.05,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
ATO J238.7552-29.9681 20260420.4247 11.73CV 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
ATO J245.2887-27.8950,2461150.9247,11.46,0.05,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
ATO J245.2887-27.8950 20260420.4247 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 6234730180787692544,2461150.9247,11.57,0.05,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 6234730180787692544 20260420.4247 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
VARIABLE_NAME,2461150.9247,11.72,0.05,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
VARIABLE_NAME 20260420.4247 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 6030853679584654976,2461150.9247,11.82,0.05,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 6030853679584654976 20260420.4247 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 6240740935981599872,2461150.9247,11.20,0.05,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 6240740935981599872 20260420.4247 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 6236663431466957056,2461150.9247,11.45,0.05,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 6236663431466957056 20260420.4247 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 6044844557036772608,2461150.9247,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6044844557036772608 20260420.4247 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046357141447015552,2461150.9247,11.44,0.05,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 6046357141447015552 20260420.4247 11.44CV 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
ATO J237.9585-28.9566,2461150.9247,11.64,0.05,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
ATO J237.9585-28.9566 20260420.4247 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 6040747364392365696,2461150.9247,11.74,0.05,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 6040747364392365696 20260420.4247 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 J249.2809-29.8858,2461150.9247,11.57,0.05,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
ATO J249.2809-29.8858 20260420.4247 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 6233885584060466944,2461150.9247,11.72,0.05,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 6233885584060466944 20260420.4247 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 6032680174562776576,2461150.9247,11.40,0.05,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 6032680174562776576 20260420.4247 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 6233242197960708608,2461150.9247,11.62,0.05,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
Gaia DR3 6233242197960708608 20260420.4247 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
Gaia DR3 6234840097591410048,2461150.9247,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6234840097591410048 20260420.4247 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6247619789961523328,2461150.9247,11.10,0.05,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 6247619789961523328 20260420.4247 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
ATO J240.9651-27.6830,2461150.9247,11.52,0.05,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
ATO J240.9651-27.6830 20260420.4247 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233008001982274304,2461150.9247,11.69,0.05,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 6233008001982274304 20260420.4247 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 6040998877679436032,2461150.9247,11.53,0.05,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 6040998877679436032 20260420.4247 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 6032212783363453696,2461150.9247,11.46,0.05,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 6032212783363453696 20260420.4247 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 6040854807295519488,2461150.9247,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6040854807295519488 20260420.4247 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6028021685566613632,2461150.9247,11.54,0.05,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 6028021685566613632 20260420.4247 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 6233331876877658880,2461150.9247,11.51,0.05,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 6233331876877658880 20260420.4247 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 6233518518974463616,2461150.9247,11.40,0.05,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 6233518518974463616 20260420.4247 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 6233521508272185472,2461150.9247,11.53,0.05,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 6233521508272185472 20260420.4247 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
ASAS J155938-2110.6,2461150.9247,10.84,0.05,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
ASAS J155938-2110.6 20260420.4247 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 6233004188051278080,2461150.9247,11.51,0.05,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 6233004188051278080 20260420.4247 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
ASAS J160733-2941.3,2461150.9247,11.57,0.05,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
ASAS J160733-2941.3 20260420.4247 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
ASAS J154542-2544.6,2461150.9247,11.46,0.05,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
ASAS J154542-2544.6 20260420.4247 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 6027912520340953728,2461150.9247,11.54,0.05,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 6027912520340953728 20260420.4247 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 6031036340283176448,2461150.9247,11.34,0.05,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 6031036340283176448 20260420.4247 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 6233461894125469056,2461150.9247,11.39,0.05,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 6233461894125469056 20260420.4247 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 6032581463380646528,2461150.9247,11.39,0.05,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 6032581463380646528 20260420.4247 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
ASASSN-V J155344.80-271625.8,2461150.9247,11.19,0.05,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
ASASSN-V J155344.80-271625.8 20260420.4247 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 J154655-2216.2,2461150.9247,10.94,0.05,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
ASAS J154655-2216.2 20260420.4247 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 6031031907875967744,2461150.9247,11.44,0.05,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 6031031907875967744 20260420.4247 11.44CV 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 6233054559427770880,2461150.9247,11.34,0.05,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 6233054559427770880 20260420.4247 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 6016802092783602944,2461150.9247,11.47,0.05,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 6016802092783602944 20260420.4247 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 6031322900467983744,2461150.9247,11.29,0.05,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 6031322900467983744 20260420.4247 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 4125716657946147328,2461150.9247,10.90,0.05,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 4125716657946147328 20260420.4247 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 6033742307119756416,2461150.9247,11.09,0.05,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 6033742307119756416 20260420.4247 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 6029570622597968256,2461150.9247,11.16,0.05,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 6029570622597968256 20260420.4247 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 6233487148533292288,2461150.9247,11.12,0.05,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 6233487148533292288 20260420.4247 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
ASAS J164710-3111.1,2461150.9247,11.13,0.05,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
ASAS J164710-3111.1 20260420.4247 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 6032677292686339072,2461150.9247,11.01,0.05,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 6032677292686339072 20260420.4247 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
ATO J236.2632-30.1380,2461150.9247,10.98,0.05,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
ATO J236.2632-30.1380 20260420.4247 10.98CV 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 6032039163597381248,2461150.9247,9.85,0.05,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 6032039163597381248 20260420.4247 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
Gaia DR3 6046778701081292160,2461150.9247,9.93,0.05,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 6046778701081292160 20260420.4247 9.93CV 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 6025800878211901568,2461150.9247,10.46,0.05,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 6025800878211901568 20260420.4247 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
ATO J237.3737-20.5227,2461150.9247,10.11,0.05,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
ATO J237.3737-20.5227 20260420.4247 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 6027987119679306624,2461150.9247,10.72,0.05,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 6027987119679306624 20260420.4247 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 6032187185354214400,2461150.9247,10.63,0.05,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 6032187185354214400 20260420.4247 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
ASAS J161949-2217.2,2461150.9247,10.36,0.05,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
ASAS J161949-2217.2 20260420.4247 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
ASASSN-V J165047.94-300805.9,2461150.9247,10.82,0.05,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
ASASSN-V J165047.94-300805.9 20260420.4247 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 6038764876213759232,2461150.9247,10.83,0.05,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
Gaia DR3 6038764876213759232 20260420.4247 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 4129909576813794304,2461150.9247,10.32,0.05,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
Gaia DR3 4129909576813794304 20260420.4247 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 6045003848780721664,2461150.9247,10.69,0.05,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 6045003848780721664 20260420.4247 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 4126652200594182144,2461150.9247,10.62,0.05,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 4126652200594182144 20260420.4247 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 6030953705118732928,2461150.9247,10.99,0.05,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 6030953705118732928 20260420.4247 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 6033815355923758720,2461150.9247,10.80,0.05,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 6033815355923758720 20260420.4247 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 6032901932308260480,2461150.9247,10.78,0.05,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 6032901932308260480 20260420.4247 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 6034641054789192064,2461150.9247,10.73,0.05,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 6034641054789192064 20260420.4247 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 6042833137954581760,2461150.9247,10.88,0.05,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 6042833137954581760 20260420.4247 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 203585851,2461150.9247,10.78,0.05,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
EPIC 203585851 20260420.4247 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 6044090085905116160,2461150.9247,10.82,0.05,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 6044090085905116160 20260420.4247 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 6032924918994623360,2461150.9247,10.92,0.05,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 6032924918994623360 20260420.4247 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 6028033642743268608,2461150.9247,10.97,0.05,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 6028033642743268608 20260420.4247 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
ATO J252.2726-28.2362,2461150.9247,10.74,0.05,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
ATO J252.2726-28.2362 20260420.4247 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
ATO J253.1776-26.6058,2461150.9247,10.88,0.05,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
ATO J253.1776-26.6058 20260420.4247 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
ASASSN-V J164726.82-235813.5,2461150.9247,10.60,0.05,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
ASASSN-V J164726.82-235813.5 20260420.4247 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 6233794565116286464,2461150.9247,11.09,0.05,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 6233794565116286464 20260420.4247 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
EPIC 204124270,2461150.9247,10.61,0.05,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
EPIC 204124270 20260420.4247 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033025116307628800,2461150.9247,10.88,0.05,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 6033025116307628800 20260420.4247 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 203914521,2461150.9247,10.84,0.05,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
EPIC 203914521 20260420.4247 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
ATO J252.1024-26.0870,2461150.9247,10.96,0.05,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
ATO J252.1024-26.0870 20260420.4247 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 6049598226836647936,2461150.9247,10.87,0.05,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 6049598226836647936 20260420.4247 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 6046647992325833344,2461150.9247,10.89,0.05,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 6046647992325833344 20260420.4247 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 6236575298740736768,2461150.9247,11.04,0.05,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 6236575298740736768 20260420.4247 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
VARIABLE_NAME,2461150.9247,11.01,0.05,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
VARIABLE_NAME 20260420.4247 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 6032090733247694592,2461150.9247,11.12,0.05,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 6032090733247694592 20260420.4247 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 6034093360554137472,2461150.9247,11.03,0.05,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 6034093360554137472 20260420.4247 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 6047017776131127296,2461150.9247,10.81,0.05,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 6047017776131127296 20260420.4247 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
ATO J252.9004-29.9367,2461150.9247,11.18,0.05,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
ATO J252.9004-29.9367 20260420.4247 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 6032672516681930496,2461150.9247,11.09,0.05,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 6032672516681930496 20260420.4247 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 6032018066717532160,2461150.9247,11.15,0.05,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 6032018066717532160 20260420.4247 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 4125619278139369728,2461150.9247,10.88,0.05,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 4125619278139369728 20260420.4247 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 6031126878203090560,2461150.9247,11.29,0.05,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 6031126878203090560 20260420.4247 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
ASASSN-V J164907.53-231125.3,2461150.9247,10.77,0.05,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
ASASSN-V J164907.53-231125.3 20260420.4247 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 6032800644167503488,2461150.9247,11.32,0.05,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 6032800644167503488 20260420.4247 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 6028033054306238080,2461150.9247,11.19,0.05,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 6028033054306238080 20260420.4247 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 4125536368096456192,2461150.9247,10.82,0.05,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 4125536368096456192 20260420.4247 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 4125657834075475200,2461150.9247,10.74,0.05,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 4125657834075475200 20260420.4247 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
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 11.13 16:43:51.55 -26:43:04.5
353.87628 12.41657 galactic Sco Second-epoch detections are separated by 6.8" and 7.5 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 6034118718041229952 | 16:43:53.24 -26:43:07.9 (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 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 6034118718041229952,2461150.9247,11.13,0.05,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
Large-amplitude variable Gaia DR2 6034118718041229952 20260420.4247 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 6034616728094251648,2461150.9247,11.01,0.05,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 6034616728094251648 20260420.4247 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 6031225142718938368,2461150.9247,11.28,0.05,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 6031225142718938368 20260420.4247 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 6033115207536998144,2461150.9247,11.15,0.05,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 6033115207536998144 20260420.4247 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 6246846146093019008,2461150.9247,10.88,0.05,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 6246846146093019008 20260420.4247 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
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 11.04 16:51:59.48 -21:28:54.4
359.28153 14.20343 galactic Oph Second-epoch detections are separated by 7.9" and 6.8 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 4127065861780781184 | 16:51:58.97 -21:28:58.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 4127065861780781184,2461150.9247,11.04,0.05,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
Large-amplitude variable Gaia DR2 4127065861780781184 20260420.4247 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
ASAS J164418-2206.8,2461150.9247,10.96,0.05,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
ASAS J164418-2206.8 20260420.4247 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
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 11.33 16:21:15.19 -29:00:33.2
348.71826 14.66615 galactic Sco Second-epoch detections are separated by 2.2" and 6.8 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 6038924889508958080 | 16:21:14.16 -29:00:58.2 (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 6038924889508958080,2461150.9247,11.33,0.05,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
Large-amplitude variable Gaia DR2 6038924889508958080 20260420.4247 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 6052089063048268672,2461150.9247,10.91,0.05,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 6052089063048268672 20260420.4247 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 6034566627278453632,2461150.9247,11.31,0.05,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 6034566627278453632 20260420.4247 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 6246711490279117312,2461150.9247,10.82,0.05,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 6246711490279117312 20260420.4247 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
ASAS J164704-2548.3,2461150.9247,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J164704-2548.3 20260420.4247 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 6031337292902555520,2461150.9247,11.51,0.05,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 6031337292902555520 20260420.4247 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 6046824227732749568,2461150.9247,11.05,0.05,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 6046824227732749568 20260420.4247 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 6028062058273943680,2461150.9247,11.47,0.05,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 6028062058273943680 20260420.4247 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
ATO J253.0086-28.0057,2461150.9247,11.30,0.05,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 J253.0086-28.0057 20260420.4247 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 6033865349333699456,2461150.9247,11.44,0.05,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 6033865349333699456 20260420.4247 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9247,11.06,0.05,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
VARIABLE_NAME 20260420.4247 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 6037507790826859392,2461150.9247,11.57,0.05,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 6037507790826859392 20260420.4247 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 6032690864784481664,2461150.9247,11.46,0.05,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 6032690864784481664 20260420.4247 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 6030893949221116288,2461150.9247,11.56,0.05,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 6030893949221116288 20260420.4247 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
ATO J246.7118-30.6081,2461150.9247,11.51,0.05,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
ATO J246.7118-30.6081 20260420.4247 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
VARIABLE_NAME,2461150.9247,11.45,0.05,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
VARIABLE_NAME 20260420.4247 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 6039956540659158528,2461150.9247,11.56,0.05,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 6039956540659158528 20260420.4247 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 6040936377314605696,2461150.9247,11.56,0.05,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 6040936377314605696 20260420.4247 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 6244055448144992256,2461150.9247,10.99,0.05,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 6244055448144992256 20260420.4247 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
ATO J253.2666-28.5934,2461150.9247,11.52,0.05,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
ATO J253.2666-28.5934 20260420.4247 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6047000763757881344,2461150.9247,11.17,0.05,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 6047000763757881344 20260420.4247 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 6246736229290838656,2461150.9247,11.16,0.05,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 6246736229290838656 20260420.4247 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 6032632040905115008,2461150.9247,11.54,0.05,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 6032632040905115008 20260420.4247 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 4125842719522931712,2461150.9247,11.14,0.05,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 4125842719522931712 20260420.4247 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
Gaia DR3 6032090733247694592,2461150.9247,11.56,0.05,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 6032090733247694592 20260420.4247 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
ATO J241.1091-21.2798,2461150.9247,11.27,0.05,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
ATO J241.1091-21.2798 20260420.4247 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
EPIC 204127444,2461150.9247,11.22,0.05,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
EPIC 204127444 20260420.4247 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 6033929842567706880,2461150.9247,11.54,0.05,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 6033929842567706880 20260420.4247 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 6234012096619068160,2461150.9247,11.47,0.05,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 6234012096619068160 20260420.4247 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
ASAS J163731-2832.0,2461150.9247,11.54,0.05,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
ASAS J163731-2832.0 20260420.4247 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 6031371416452919168,2461150.9247,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6031371416452919168 20260420.4247 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202842956,2461150.9247,11.57,0.05,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
EPIC 202842956 20260420.4247 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
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 11.62 16:46:02.78 -29:37:25.3
351.89768 10.20027 galactic Sco Second-epoch detections are separated by 4.3" and 7.1 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 6031329531927978880 | 16:46:04.17 -29:37:29.1 (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 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 6031329531927978880,2461150.9247,11.62,0.05,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
Large-amplitude variable Gaia DR2 6031329531927978880 20260420.4247 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
Gaia DR3 4127004426577825664,2461150.9247,11.34,0.05,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 4127004426577825664 20260420.4247 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 6025800775132667520,2461150.9247,11.70,0.05,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 6025800775132667520 20260420.4247 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
ATO J245.9869-26.6598,2461150.9247,11.51,0.05,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
ATO J245.9869-26.6598 20260420.4247 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 6234088924994491520,2461150.9247,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6234088924994491520 20260420.4247 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J160330.34-251111.3,2461150.9247,11.49,0.05,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
ASASSN-V J160330.34-251111.3 20260420.4247 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 4126537890054326272,2461150.9247,11.43,0.05,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 4126537890054326272 20260420.4247 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
CW Sco,2461150.9247,11.73,0.05,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
CW Sco 20260420.4247 11.73CV 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 4126466589287514752,2461150.9247,11.38,0.05,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 4126466589287514752 20260420.4247 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
EPIC 204379265,2461150.9247,11.36,0.05,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
EPIC 204379265 20260420.4247 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
EPIC 204280860,2461150.9247,11.35,0.05,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
EPIC 204280860 20260420.4247 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 6242364674142405376,2461150.9247,11.41,0.05,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 6242364674142405376 20260420.4247 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 6031906260107794688,2461150.9247,11.76,0.05,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 6031906260107794688 20260420.4247 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 6037918046102425728,2461150.9247,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6037918046102425728 20260420.4247 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032927706446179968,2461150.9247,11.77,0.05,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 6032927706446179968 20260420.4247 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
Gaia DR3 6242465485608147840,2461150.9247,11.40,0.05,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 6242465485608147840 20260420.4247 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 6048539534578287360,2461150.9247,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6048539534578287360 20260420.4247 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233704302084209920,2461150.9247,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6233704302084209920 20260420.4247 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6242184487367615872,2461150.9247,11.43,0.05,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 6242184487367615872 20260420.4247 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
ATO J251.3841-29.3388,2461150.9247,11.78,0.05,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
ATO J251.3841-29.3388 20260420.4247 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
V0898 Sco,2461150.9247,11.82,0.05,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
V0898 Sco 20260420.4247 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 6033912692735505920,2461150.9247,11.61,0.05,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 6033912692735505920 20260420.4247 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
Gaia DR3 6039853942478154368,2461150.9247,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6039853942478154368 20260420.4247 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J244.9171-28.9991,2461150.9247,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J244.9171-28.9991 20260420.4247 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126568332777777408,2461150.9247,11.46,0.05,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 4126568332777777408 20260420.4247 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
EPIC 202607322,2461150.9247,11.85,0.05,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
EPIC 202607322 20260420.4247 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 6242153838482448384,2461150.9247,11.49,0.05,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 6242153838482448384 20260420.4247 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
ASASSN-V J164247.78-284800.2,2461150.9247,11.86,0.05,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
ASASSN-V J164247.78-284800.2 20260420.4247 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 4125859628820417024,2461150.9247,11.52,0.05,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 4125859628820417024 20260420.4247 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6039951867734597248,2461150.9247,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6039951867734597248 20260420.4247 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6025494492429646848,2461150.9247,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6025494492429646848 20260420.4247 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6235734000546171776,2461150.9247,11.85,0.05,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 6235734000546171776 20260420.4247 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
ASASSN-V J163912.98-232902.9,2461150.9247,11.61,0.05,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
ASASSN-V J163912.98-232902.9 20260420.4247 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
Gaia DR3 6030871203053970560,2461150.9247,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030871203053970560 20260420.4247 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031452367978522112,2461150.9247,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6031452367978522112 20260420.4247 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040144866387906048,2461150.9247,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6040144866387906048 20260420.4247 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.4262-25.3128,2461150.9247,11.95,0.05,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
ATO J241.4262-25.3128 20260420.4247 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
ATO J240.9666-27.6064,2461150.9247,11.90,0.05,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
ATO J240.9666-27.6064 20260420.4247 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
ATO J240.9648-24.9799,2461150.9247,11.74,0.05,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
ATO J240.9648-24.9799 20260420.4247 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 J238.3783-29.7159,2461150.9247,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J238.3783-29.7159 20260420.4247 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4247 2461150.9247 12.11 15:46:29.73 -26:29:16.5
344.76188 21.83274 galactic Lib Second-epoch detections are separated by 8.4" and 6.3 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 6234734166517538048 | 15:46:28.08 -26:29:25.9 (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 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 6234734166517538048,2461150.9247,12.11,0.05,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
Large-amplitude variable Gaia DR2 6234734166517538048 20260420.4247 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
ATO J241.0955-27.3357,2461150.9247,12.07,0.05,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
ATO J241.0955-27.3357 20260420.4247 12.07CV 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 6043396637662959872,2461150.9247,12.01,0.05,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 6043396637662959872 20260420.4247 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 6044623138577197568,2461150.9247,12.06,0.05,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 6044623138577197568 20260420.4247 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037027613487393664,2461150.9247,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6037027613487393664 20260420.4247 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6047207716762276096,2461150.9247,11.81,0.05,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 6047207716762276096 20260420.4247 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 6234101500658776960,2461150.9247,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6234101500658776960 20260420.4247 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J242.0313-30.2439,2461150.9247,11.60,0.05,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
ATO J242.0313-30.2439 20260420.4247 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 6236740122403156352,2461150.9247,11.38,0.05,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 6236740122403156352 20260420.4247 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
ASASSN-V J162319.11-295356.1,2461150.9247,11.85,0.05,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
ASASSN-V J162319.11-295356.1 20260420.4247 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 6033050228939081088,2461150.9247,11.76,0.05,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 6033050228939081088 20260420.4247 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 J163913.26-302421.4,2461150.9247,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J163913.26-302421.4 20260420.4247 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 6040444788234836480,2461150.9247,11.69,0.05,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 6040444788234836480 20260420.4247 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
EPIC 204477108,2461150.9247,11.13,0.05,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
EPIC 204477108 20260420.4247 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 6031311733554619520,2461150.9247,11.89,0.05,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 6031311733554619520 20260420.4247 11.89CV 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 6031125843075056384,2461150.9247,11.03,0.05,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 6031125843075056384 20260420.4247 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
ATO J253.1610-28.6129,2461150.9247,10.98,0.05,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
ATO J253.1610-28.6129 20260420.4247 10.98CV 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 6043626126357774464,2461150.9247,11.85,0.05,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 6043626126357774464 20260420.4247 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 6038761921275553024,2461150.9247,12.06,0.05,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 6038761921275553024 20260420.4247 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046197742307386240,2461150.9247,11.13,0.05,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 6046197742307386240 20260420.4247 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 J160926.47-305707.1,2461150.9247,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J160926.47-305707.1 20260420.4247 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032266208433826560,2461150.9247,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6032266208433826560 20260420.4247 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031147872005817856,2461150.9247,11.40,0.05,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 6031147872005817856 20260420.4247 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 6243852279007998208,2461150.9247,10.54,0.05,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 6243852279007998208 20260420.4247 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032914203067481984,2461150.9247,10.24,0.05,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 6032914203067481984 20260420.4247 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 6032582592900505344,2461150.9247,11.62,0.05,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
Gaia DR3 6032582592900505344 20260420.4247 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
WISE J162318.4-303811,2461150.9247,11.62,0.05,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
WISE J162318.4-303811 20260420.4247 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
ATO J238.2149-27.4201,2461150.9247,11.49,0.05,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
ATO J238.2149-27.4201 20260420.4247 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
ATO J244.3965-21.1528,2461150.9247,10.47,0.05,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
ATO J244.3965-21.1528 20260420.4247 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
ATO J241.7560-28.0375,2461150.9247,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J241.7560-28.0375 20260420.4247 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164755-2809.5,2461150.9247,10.85,0.05,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
ASAS J164755-2809.5 20260420.4247 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
ASASSN-V J164907.36-272443.3,2461150.9247,11.21,0.05,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
ASASSN-V J164907.36-272443.3 20260420.4247 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J155700.97-285630.5,2461150.9247,11.96,0.05,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
ASASSN-V J155700.97-285630.5 20260420.4247 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
BB Sco,2461150.9247,11.29,0.05,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
BB Sco 20260420.4247 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 6037509298350592384,2461150.9247,11.94,0.05,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 6037509298350592384 20260420.4247 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 6034178705826271872,2461150.9247,11.49,0.05,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 6034178705826271872 20260420.4247 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
ATO J253.3405-29.8117,2461150.9247,11.90,0.05,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
ATO J253.3405-29.8117 20260420.4247 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
ATO J253.1022-25.9063,2461150.9247,10.80,0.05,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
ATO J253.1022-25.9063 20260420.4247 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 6044614484233409920,2461150.9247,11.43,0.05,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 6044614484233409920 20260420.4247 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
ATO J246.8152-26.0183,2461150.9247,11.25,0.05,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
ATO J246.8152-26.0183 20260420.4247 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 6039206330125563904,2461150.9247,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6039206330125563904 20260420.4247 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040896726175962496,2461150.9247,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6040896726175962496 20260420.4247 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6043114406769759232,2461150.9247,11.62,0.05,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
Gaia DR3 6043114406769759232 20260420.4247 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
ATO J252.5528-29.7410,2461150.9247,11.78,0.05,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
ATO J252.5528-29.7410 20260420.4247 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 6032698282139528320,2461150.9247,10.84,0.05,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 6032698282139528320 20260420.4247 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 6034172559750580736,2461150.9247,11.88,0.05,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
Gaia DR3 6034172559750580736 20260420.4247 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 6030976416907416704,2461150.9247,11.60,0.05,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 6030976416907416704 20260420.4247 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 6046933869646677504,2461150.9247,11.45,0.05,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 6046933869646677504 20260420.4247 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 6032220067619988096,2461150.9247,10.88,0.05,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 6032220067619988096 20260420.4247 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 6048248915610902912,2461150.9247,10.14,0.05,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 6048248915610902912 20260420.4247 10.14CV 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
Gaia DR3 6032982475860717824,2461150.9247,10.66,0.05,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 6032982475860717824 20260420.4247 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 6040577008812557184,2461150.9247,11.49,0.05,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 6040577008812557184 20260420.4247 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
ATO J242.0224-28.7894,2461150.9247,11.73,0.05,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
ATO J242.0224-28.7894 20260420.4247 11.73CV 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 6032218349639104512,2461150.9247,11.11,0.05,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 6032218349639104512 20260420.4247 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 6246855869898980992,2461150.9247,10.37,0.05,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 6246855869898980992 20260420.4247 10.37CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.92510688 20.04.2026 10:11:59.234 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8315
Objects passed selection criteria: 8275
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 5603.75
Average stars matched: 5397.5 (96.3194 %)
Memory usage VmPeak: 114064 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 05:14:00 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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.92510688 20.04.2026 10:11:59.234 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 648
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.99
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: 16 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): 77511
Objects passed selection criteria: 77319
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 50265
Average stars matched: 47639 (94.7757 %)
Memory usage VmPeak: 176744 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 05:16:18 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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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: 2461150.92438853
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits'
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 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-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Image size: 942.0'x627.8' 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: 16:19:12.163 -26:00:43.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:12.163 -26:00:43.47
Angular distance between the image centers 0.0247 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Image size: 942.0'x627.8' 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: 16:19:14.130 -26:00:10.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:14.130 -26:00:10.56
Angular distance between the image centers 0.0130 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 16:19:12.163 -26:00:43.47
Second-epoch second image center 16:19:14.130 -26:00:10.56
Angular distance between the image centers 0.01174 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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.8HGivvGrk7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.fz58sePmIv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits &> /tmp/tmp.uJJ1crbluk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits &> /tmp/tmp.pDCnTtd1Kz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 8752 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 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 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 deg
Loaded 8190 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): 5578 out of 5823 total matches.
Matched with Tycho-2 5823 out of 8752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802561
a=0.000000 b=1.000000 c=22.802561
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.2 pix Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
9.8 pix fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
9.8 pix fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
12.7 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
12.7 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.4 (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.8HGivvGrk7 (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=8752
Got 8752 stars (including 8042 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 8752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
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: 962 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.fz58sePmIv (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=689, passed=8852
Got 8852 stars (including 8148 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 8852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
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: 960 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 293 to 349 (Dec -31.3 to -20.4)
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(), 8677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 960 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-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.uJJ1crbluk (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=587, passed=2668
Got 2668 stars (including 2081 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat
util/solve_plate_with_UCAC5 got 2668 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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 959 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(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.44"
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 292 to 351 (Dec -31.5 to -20.0)
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(), 2587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.18"
Excluding outliers - 956 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_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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.pDCnTtd1Kz (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=668, passed=2790
Got 2790 stars (including 2122 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat
util/solve_plate_with_UCAC5 got 2790 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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.47"
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 292 to 351 (Dec -31.5 to -20.0)
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: 954 matched stars entering correct_measured_positions(), 2686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.37"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 2685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.19"
Excluding outliers - 954 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits'
Preparing the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
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__out20622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20747.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
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: 10s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20616_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20616_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20617_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20617_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20619_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20619_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20620_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20620_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20622_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20622_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:20:21.63 -25:06:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.45, MAG_FAINT_SEARCH_LIMIT=10.43)GAIADR2_OUTPUT=# 1.254 6048821593667585536 245.08977417692 -25.11500419561 8.4399 7.5614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20640_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20640_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:15.30 -21:40:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.02, MAG_FAINT_SEARCH_LIMIT=10.00)GAIADR2_OUTPUT=# 1.995 4127001540359719424 253.31341790164 -21.67487696011 7.5751 6.2190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20653_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20653_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:29.92 -21:39:23.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20665_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20665_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20674_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20674_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20681_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20681_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20697_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20697_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20702_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20702_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20704_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20704_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20706_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20706_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:39.76 -21:45:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.25, MAG_FAINT_SEARCH_LIMIT=11.23)GAIADR2_OUTPUT=# 3.275 4126993740699126784 253.16498858559 -21.76201743639 9.1964 8.1841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20711_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20711_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20715_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20715_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20719_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20719_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20720_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20720_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20721_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20721_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20728_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20728_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:39.46 -21:45:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 3.278 4126993740699126784 253.16498858559 -21.76201743639 9.1964 8.1841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20730_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20730_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20743_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20743_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20746_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20746_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20747_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 20747_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01392_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 01392_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:00:42.41 -29:55:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04757_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 04757_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05578_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 05578_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:21:10.99 -25:35:31.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06622_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 06622_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:20:37.95 -24:10:12.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04509_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 04509_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:29:24.01 -26:25:52.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03563_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 03563_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:12:18.45 -27:55:27.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02916_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 02916_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:18:17.87 -28:36:44.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06022_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 06022_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:30:11.91 -25:06:55.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04856_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 04856_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:08:08.08 -26:19:33.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06970_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 06970_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:25:34.64 -23:26:53.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05284_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 05284_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:03:20.94 -25:51:53.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 02018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:11:02.08 -29:24:53.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03269_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 03269_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:35:52.15 -28:12:48.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05009_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 05009_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:58:51.75 -26:06:45.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05631_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 05631_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:53:37.16 -25:19:36.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05250_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 05250_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:59.14 -25:45:03.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02052_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 02052_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:56:53.49 -29:12:43.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08272_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 08272_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:07:24.59 -20:52:13.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07316_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 07316_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:00:20.41 -22:37:21.8 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 43s
Prepared the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:23:35.42 -26:31:37.7
16:52:09.48 -28:12:42.5
16:53:14.38 -29:31:09.5
16:50:23.00 -28:32:20.9
16:43:06.15 -21:41:24.0
16:44:19.94 -26:19:30.5
16:24:16.94 -31:10:22.5
16:46:15.66 -29:09:41.6
16:43:46.69 -25:13:32.6
16:13:23.98 -21:58:10.0
16:51:43.72 -23:54:10.9
16:48:52.24 -28:26:08.4
16:46:54.24 -30:07:53.4
16:45:20.68 -26:54:43.3
16:49:51.34 -24:26:52.8
16:43:43.36 -30:45:03.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 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-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Image size: 942.0'x627.8' 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: 16:19:12.163 -26:00:43.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:12.163 -26:00:43.47
Angular distance between the image centers 0.0247 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Image size: 942.0'x627.8' 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: 16:19:14.130 -26:00:10.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:14.130 -26:00:10.56
Angular distance between the image centers 0.0130 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 16:19:12.163 -26:00:43.47
Second-epoch second image center 16:19:14.130 -26:00:10.56
Angular distance between the image centers 0.01174 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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.3AIooQs9Ec
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.fHqSYDT4K0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits &> /tmp/tmp.3bV0V7Xgyo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits &> /tmp/tmp.ytPjzOFa2x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 85371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 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 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 deg
Loaded 8263 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): 6163 out of 6991 total matches.
Matched with Tycho-2 6991 out of 85371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.625106
a=0.000000 b=1.000000 c=22.625106
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.64
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 504 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.0 pix Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
4.3 pix fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
4.3 pix fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
12.9 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
12.9 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3AIooQs9Ec (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4769, passed=85362
Got 85362 stars (including 80423 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 85362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.fHqSYDT4K0 (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4773, passed=84608
Got 84608 stars (including 79674 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 84608 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.3bV0V7Xgyo (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4739, passed=17110
Got 17110 stars (including 12355 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat
util/solve_plate_with_UCAC5 got 17110 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 292 to 351 (Dec -31.6 to -20.0)
Done reading UCAC5 zone files...
Matched 960 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(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 16685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.28"
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 292 to 351 (Dec -31.6 to -20.0)
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: 957 matched stars entering correct_measured_positions(), 16685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.26"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 16685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.07"
Excluding outliers - 957 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_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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.ytPjzOFa2x (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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=4734, passed=17399
Got 17399 stars (including 12647 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat
util/solve_plate_with_UCAC5 got 17399 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 292 to 351 (Dec -31.6 to -20.0)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 16788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.29"
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 292 to 351 (Dec -31.6 to -20.0)
Done reading UCAC5 zone files...
Matched 959 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(), 16787 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.28"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16787 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.08"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-10-57_20.00sec_-4.90C_LIGHTs_0008.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.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-02-Q1b1x1_051258_TTUQ1b1x1_1592427_kh8geox6/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009.fits
Preparing the HTML report for the field Sco-02-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
Adding exclusion_list_gaiadr2.txt__out103020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out12444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out103313.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out103434.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out02680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95860.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 378s
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: 191s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103001_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103001_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103003_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103003_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103013_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103013_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103020_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103020_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:51:08.00 -20:41:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 2.908 6246869819952873856 237.78259830377 -20.68813150869 12.2141 11.4951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103021_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103021_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103024_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103024_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103026_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103026_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:41:42.35 -24:40:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 5.589 6047019421095811840 250.42765152347 -24.67705534214 11.2096 10.2124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103031_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103031_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103033_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103033_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103036_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103036_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103038_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103038_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:42.87 -20:34:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.731 6247622263862705536 237.67866627816 -20.57620151311 11.8887 11.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103045_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103045_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:16.78 -24:30:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.831 4113290183701683712 253.31961854678 -24.50909690433 11.1816 10.1216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103047_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103047_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103053_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103053_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103055_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103055_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:02.17 -29:29:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.898 6233058064121143552 235.76018840223 -29.48785797910 11.9490 11.1669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103057_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103057_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103061_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103061_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103068_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103068_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103075_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103075_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:16.62 -28:02:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.556 6233577789526444672 237.56909460607 -28.04582114332 11.5372 10.5975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103076_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103076_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103077_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103077_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103081_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103081_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:42.26 -29:00:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.708 6233087132459953280 235.92526980109 -29.00227270484 12.1321 11.6128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103085_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103085_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:10.88 -21:11:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 3.082 6240834325744385664 237.54479216028 -21.18414178094 11.7024 11.1291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103091_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103091_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:48:55.88 -30:09:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103093_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103093_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103094_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103094_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:51:44.15 -20:48:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 4.763 6246852571364140160 237.93288946926 -20.81460496654 11.7672 10.9955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103095_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103095_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103101_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103101_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103102_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103102_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:45:50.61 -25:36:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.262 6235105354767344256 236.46057895572 -25.60754095909 10.9220 9.7393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103106_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103106_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103108_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103108_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:30:13.94 -29:54:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.391 6043831494512483072 247.55738088318 -29.90115166286 11.5513 10.6719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103109_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103109_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103110_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103110_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103115_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103115_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103118_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103118_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:15.89 -29:19:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 5.712 6233072563930787584 235.81452623078 -29.31877171763 11.7378 11.2557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103120_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103120_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:45:37.06 -30:01:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103121_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103121_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103125_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103125_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:07:41.66 -28:39:53.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103143_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103143_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103145_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103145_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103156_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103156_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103166_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103166_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103167_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103167_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103169_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103169_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103177_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103177_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:44:29.46 -29:19:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 4.095 6031398251410785152 251.12404411468 -29.32735536619 11.9286 11.1814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103183_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103183_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:33.87 -28:17:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 5.733 6233380633345899264 235.88931998112 -28.28882207768 11.6520 10.9231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103184_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103184_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103185_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103185_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:22.77 -30:08:21.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103194_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103194_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:22.90 -20:59:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 5.248 6240855761925181824 237.59548365992 -20.99573808399 11.3019 10.5509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103200_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103200_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103205_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103205_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103206_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103206_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103208_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103208_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103209_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103209_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103213_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103213_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103216_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103216_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103217_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103217_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:22:16.03 -25:20:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.542 6048986967088604288 245.56657703367 -25.34278474371 10.5715 9.6627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103222_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103222_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103231_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103231_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103233_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103233_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:10:21.07 -24:32:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 5.730 6049848125214441344 242.58613540658 -24.54287553032 10.5165 9.5308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103236_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103236_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103238_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103238_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:49:24.05 -21:05:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 4.021 6240851093301983232 237.34901352952 -21.09506719513 11.1372 10.2646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103239_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103239_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103242_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103242_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:03:34.71 -22:04:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 5.711 6243339562991739520 240.89336327823 -22.07737227199 10.6677 9.7006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103243_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103243_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:45:33.47 -28:35:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.110 6233217527668312192 236.38849141691 -28.58468759763 11.7353 11.0452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103244_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103244_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103251_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103251_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:04:35.81 -29:44:06.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103252_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103252_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103253_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103253_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:45:14.75 -30:00:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103254_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103254_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103255_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103255_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103257_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103257_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103258_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103258_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103265_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103265_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103269_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103269_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:03.92 -25:45:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.113 6034651465791694848 252.51760183040 -25.75116646169 10.6461 9.8824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103272_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103272_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103276_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103276_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103281_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103281_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103282_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103282_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103284_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103284_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:52:21.41 -22:28:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 5.364 6240365968156366464 238.08762343405 -22.46839260832 10.5565 9.3832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103286_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103286_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103287_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103287_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103289_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103289_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103291_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103291_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103298_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103298_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103300_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103300_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:49:20.36 -30:58:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103301_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103301_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:35.83 -30:42:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103302_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103302_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:25.41 -30:22:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103303_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103303_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:51:56.06 -21:22:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.985 6240778181937372544 237.98265209336 -21.37914252528 11.2174 10.4690 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 103307_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103307_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103308_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103308_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103309_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103309_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:43:50.60 -22:12:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 4.067 4126736042657580672 250.96204416466 -22.20325053889 10.6074 9.9266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103311_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103311_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103312_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103312_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103313_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103313_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:42.67 -30:34:27.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103315_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103315_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:39:57.91 -26:01:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.783 6046406619463366144 249.99210447948 -26.03111435795 10.1683 9.1754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103320_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103320_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:58.40 -21:55:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 3.779 4126615435675162880 252.99440365199 -21.93056336080 10.9180 10.5366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103322_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103322_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103327_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103327_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103329_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103329_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:53.47 -29:54:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103335_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103335_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103336_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103336_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:52:50.26 -21:45:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 3.246 6240565907473603968 238.20856281816 -21.74987626275 10.8196 9.8560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103337_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103337_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:23.81 -28:24:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103340_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103340_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:46:20.81 -25:08:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.585 6046756504690056832 251.58835912619 -25.14538864080 10.2398 9.5047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103341_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103341_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103343_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103343_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103344_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103344_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103346_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103346_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103347_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103347_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:36.00 -29:35:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 5.603 6233052772721373824 235.89855401179 -29.58841697435 11.3393 10.5891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103351_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103351_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103355_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103355_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103359_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103359_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:39.16 -30:24:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103366_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103366_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103369_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103369_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103370_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103370_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103371_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103371_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103376_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103376_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103379_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103379_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103382_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103382_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103383_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103383_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:32.59 -29:35:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 5.255 6032595580881580928 252.88710225050 -29.59724537826 11.0990 10.3626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103385_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103385_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103387_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103387_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103388_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103388_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103392_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103392_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103394_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103394_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103396_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103396_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103400_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103400_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103401_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103401_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103402_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103402_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103403_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103403_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103404_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103404_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103406_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103406_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:18:14.94 -25:41:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 2.222 6048775070581577728 244.56166988413 -25.68764416889 9.5054 8.4006 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 103407_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103407_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:41:51.20 -25:50:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 3.078 6046319345733712256 250.46426390067 -25.83960565044 9.8020 8.7894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103409_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103409_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103412_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103412_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103415_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103415_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103419_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103419_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:19.43 -27:59:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103422_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103422_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103427_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103427_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103431_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103431_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:34.34 -30:42:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103433_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103433_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:53.52 -30:45:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103434_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103434_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:36.03 -28:34:19.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103435_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103435_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:03.86 -30:55:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103437_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103437_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103439_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103439_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103460_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103460_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103471_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103471_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:37.63 -22:42:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.62, MAG_FAINT_SEARCH_LIMIT=9.60)GAIADR2_OUTPUT=# 1.119 4125754281857815168 253.15703498542 -22.71478487457 8.2096 7.1343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103474_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103474_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103483_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103483_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:23:35.80 -26:31:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103487_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103487_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:02.03 -22:19:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.99, MAG_FAINT_SEARCH_LIMIT=9.97)GAIADR2_OUTPUT=# 3.364 4125846739612312704 253.00748651599 -22.31756004598 8.9071 8.1023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103496_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103496_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:52.89 -22:12:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.19, MAG_FAINT_SEARCH_LIMIT=10.17)GAIADR2_OUTPUT=# 1.536 4126604096961519488 252.71993845242 -22.20585872899 9.2706 8.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103501_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103501_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103504_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103504_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:02.16 -24:10:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.28, MAG_FAINT_SEARCH_LIMIT=10.26)GAIADR2_OUTPUT=# 2.415 4125326400039294592 253.25972939729 -24.16996984394 8.6065 7.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103509_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103509_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:57.56 -22:46:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.36, MAG_FAINT_SEARCH_LIMIT=10.34)GAIADR2_OUTPUT=# 0.328 4125799258758058880 252.98973446576 -22.77327798659 9.3391 8.5113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103511_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103511_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:09.07 -22:08:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.46, MAG_FAINT_SEARCH_LIMIT=10.44)GAIADR2_OUTPUT=# 0.853 4126605883667911424 252.78804597455 -22.14327449663 9.4068 8.5810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103512_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103512_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103527_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103527_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103534_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103534_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103536_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103536_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:04.83 -22:05:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.79, MAG_FAINT_SEARCH_LIMIT=10.77)GAIADR2_OUTPUT=# 2.749 4126231195034615424 253.26930339035 -22.08525205720 9.9454 9.1972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103538_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103538_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103543_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103543_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103544_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103544_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103554_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103554_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103555_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103555_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:43:46.50 -25:13:35.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103562_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103562_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:48:01.98 -22:27:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.04, MAG_FAINT_SEARCH_LIMIT=11.02)GAIADR2_OUTPUT=# 5.461 4126491023368323968 252.00958128498 -22.45822379731 9.8663 9.0797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103563_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103563_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:46:54.21 -30:07:52.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103567_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103567_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103573_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103573_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:47.42 -22:57:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 4.185 4125697072894791680 252.69884593343 -22.96487526373 9.9013 9.1216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103575_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103575_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103579_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103579_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103584_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103584_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103612_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103612_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103613_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103613_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103621_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103621_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103631_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103631_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103647_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103647_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103650_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103650_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103655_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103655_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103661_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103661_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:43.89 -24:26:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 5.034 4125301008192076800 253.18438529111 -24.43527329592 10.6716 10.2903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103662_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103662_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103670_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103670_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103674_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103674_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103680_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103680_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103696_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103696_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:28.55 -21:55:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 1.480 4126987830824033152 253.11851956946 -21.92483574425 10.4253 9.6239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103701_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103701_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103703_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103703_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103705_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103705_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103707_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103707_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103712_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103712_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103714_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103714_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103715_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103715_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103717_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103717_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103722_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103722_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103727_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103727_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103728_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103728_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103729_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103729_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103735_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103735_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103737_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103737_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:15.17 -23:21:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 3.058 4125625153657586560 253.06388706811 -23.35347836741 11.2102 10.6234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103746_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103746_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103751_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103751_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:23.39 -22:09:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 0.736 4125858288790594688 253.09749067962 -22.15115891537 10.6014 10.0224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103754_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103754_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:46:42.52 -21:51:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.960 4126850529303941888 251.67805242832 -21.86532370777 10.5289 9.5988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103756_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103756_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103758_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103758_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103760_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103760_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103761_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103761_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103762_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103762_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103784_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103784_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103786_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103786_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103788_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103788_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103792_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103792_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103800_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103800_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:25.37 -22:10:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103803_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103803_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103804_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103804_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103811_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103811_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103814_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103814_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103815_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103815_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103817_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103817_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:23.43 -22:08:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 2.021 4126218447571569536 253.34760670749 -22.14603322875 11.0200 10.4027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103821_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103821_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103823_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103823_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103830_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103830_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103833_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103833_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103835_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103835_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103837_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103837_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103844_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103844_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103848_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103848_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103849_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103849_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103854_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103854_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:27.81 -24:51:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 5.437 6046823609257443072 252.86742139968 -24.85461387517 10.8457 10.0583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103856_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103856_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103860_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103860_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:43.25 -22:56:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 1.542 4125744038350876160 252.93066686971 -22.94917797218 10.8883 9.9953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103867_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103867_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:11.74 -23:02:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 5.048 4125739301011635712 253.04913627134 -23.04730414104 11.2733 10.7060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103868_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103868_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:47.23 -22:28:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.561 4125842719522931712 252.94723663737 -22.47736031292 10.6525 9.6903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103870_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103870_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103872_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103872_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103876_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103876_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103891_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103891_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103892_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103892_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103896_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103896_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103899_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103899_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103900_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103900_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103904_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103904_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103908_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103908_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:47:35.25 -22:13:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.686 4126546166446713344 251.89767527651 -22.21738457575 11.0852 10.5067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103909_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103909_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103914_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103914_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103916_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103916_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103920_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103920_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103923_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103923_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103927_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103927_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103928_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103928_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103937_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103937_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103940_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103940_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103943_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103943_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103947_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103947_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103950_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103950_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103951_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103951_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103956_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103956_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103958_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103958_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103961_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103961_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103964_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103964_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103968_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103968_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103979_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 103979_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:51.67 -22:18:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.941 4125849350952428288 252.96514733924 -22.31380291112 11.0429 10.5485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103983_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103983_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103987_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103987_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103989_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103989_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103990_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 103990_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104002_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104002_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104003_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104003_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104009_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104009_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:53.06 -22:36:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 4.273 4125817400700271232 252.72207165193 -22.61171310274 11.2441 10.7901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104011_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104011_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104017_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104017_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:11.22 -22:37:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 0.485 4125816472987254784 252.79688048142 -22.62347718585 11.1953 10.5846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104018_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104019_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104019_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104022_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104022_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104024_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104024_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104030_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104030_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:30.28 -23:31:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 0.891 4125513072193453440 253.37592285080 -23.51736622667 10.8598 9.8781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104041_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104041_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104050_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104050_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104057_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104057_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:40.84 -22:03:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 4.191 4126609903757294208 252.92141202450 -22.05143231487 10.7183 9.8807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104058_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104058_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104063_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104063_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104064_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104064_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104069_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104069_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104072_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104072_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104074_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104074_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104080_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104080_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104081_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104081_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104084_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104084_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104090_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104090_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:05.86 -22:36:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.458 4125813926058704896 252.52487582358 -22.61202012439 10.6698 9.8652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104100_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104100_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104107_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104107_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104108_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104108_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104110_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104110_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104112_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104112_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:49:26.68 -22:10:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 4.010 4126595614410344576 252.36163363540 -22.17322342825 10.7825 9.9644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104114_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104114_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104126_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104126_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104128_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104128_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104134_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104134_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104141_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104141_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104142_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104142_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104147_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104147_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104150_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104150_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104156_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104156_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:51:17.38 -22:10:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.917 4126602795596710016 252.82253875634 -22.18039218238 10.8175 9.6808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104163_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104163_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104165_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104165_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104169_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104169_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104172_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104172_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104173_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104173_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104174_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104174_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104180_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104180_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104194_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104194_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104196_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104196_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104200_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104200_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104204_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104204_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104207_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104207_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104208_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104208_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104212_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104212_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104217_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104217_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104231_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104231_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104238_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104238_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104242_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104242_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104244_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104244_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104246_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104246_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104248_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104248_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104258_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104258_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104259_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104259_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104262_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104262_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104265_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104265_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104271_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104271_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104276_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104276_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104279_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104279_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104285_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104285_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104297_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104297_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104298_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104298_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104304_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104304_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104310_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104310_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104322_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104322_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104332_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104332_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104336_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104336_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104338_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104338_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104342_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104342_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104344_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104344_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104347_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104347_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104352_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104352_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:54:41.73 -21:04:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 4.828 6246785810386881280 238.67277657356 -21.07338491151 11.3677 10.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104354_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104354_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:56.57 -22:45:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 4.630 4125773626391520640 253.23437928431 -22.75152874217 11.3146 10.3230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104356_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104356_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104358_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104358_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104364_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104364_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104369_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104369_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104380_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104380_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:36.58 -22:46:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 5.091 4125796265153191808 252.65291982476 -22.78058592535 10.5718 9.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104381_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104381_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104382_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104382_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104404_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104404_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104406_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104406_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104407_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104407_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104411_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104411_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104415_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104415_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104426_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104426_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104429_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104429_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104441_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104441_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104451_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104451_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104469_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104469_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104471_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104471_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104473_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104473_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104491_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104491_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104506_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104506_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104512_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104512_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104530_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104530_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104532_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104532_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104550_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104550_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104554_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104554_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104557_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104557_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104559_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104559_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104572_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104572_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104583_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104583_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104592_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104592_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104595_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104595_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104600_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104600_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104608_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104608_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104630_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104630_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104643_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104643_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104654_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104654_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104661_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104661_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104666_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104666_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104669_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 104669_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104670_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104670_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:45:02.04 -28:54:21.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104697_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104697_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104769_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 104769_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95582_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 95582_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:53:04.39 -28:35:14.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95793_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 95793_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:48:21.49 -20:34:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 2.774 6241675585282641664 237.08938048392 -20.57291104806 12.0093 11.1522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95860_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 95860_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32189_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 32189_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:34.24 -27:54:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 3.544 6033099676934125056 253.14371080581 -27.91231578551 11.0687 10.2991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12444_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 12444_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:55:39.73 -29:47:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33479_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 33479_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:31:41.05 -27:54:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26638_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 26638_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:38:12.81 -28:34:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77398_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 77398_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13918_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 13918_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26077_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 26077_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:52:35.25 -28:33:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31858_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 31858_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08395_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 08395_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22210_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 22210_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77610_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 77610_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13957_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 13957_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13249_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 13249_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25597_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 25597_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57034_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 57034_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:50:55.86 -25:10:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 49349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09796_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 09796_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:46:39.77 -29:52:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 25135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47527_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 47527_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02809_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 02809_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28705_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 28705_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14266_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 14266_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60545_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 60545_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26227_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 26227_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14582_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 14582_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06353_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 06353_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57579_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 57579_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:09:51.70 -25:08:40.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35377_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 35377_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28999_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 28999_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:24:09.26 -28:22:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62071_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 62071_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31358_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 31358_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30225_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 30225_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 37099_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21315_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 21315_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14833_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 14833_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02680_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 02680_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44834_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 44834_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13178_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 13178_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50966_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 50966_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95817_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 95817_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95803_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 95803_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95610_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 95610_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95591_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 95591_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:43:56.17 -29:08:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29278_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 29278_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14192_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 14192_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13060_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 13060_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40086_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 40086_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14446_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 14446_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69181_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 69181_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:17:40.80 -22:53:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21597_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 21597_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46189_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 46189_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27176_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 27176_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05201_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 05201_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 58414_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22985_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 22985_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66847_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 66847_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29216_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 29216_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52768_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 52768_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:21:11.03 -25:35:31.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20449_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 20449_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:46:15.47 -29:09:41.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04947_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 04947_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54378_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 54378_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:14:53.44 -25:28:37.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84408_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 84408_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:13:45.48 -24:25:19.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19032_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 19032_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 81135_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:20:37.94 -24:10:13.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42152_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 42152_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:29:24.00 -26:25:52.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85178_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 85178_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:07:51.83 -24:27:45.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45130_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 45130_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:31:22.71 -26:32:16.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57619_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 57619_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:30:11.93 -25:06:55.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 24915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:18:17.87 -28:36:44.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31742_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 31742_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:12:18.47 -27:55:27.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45724_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 45724_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:08:08.13 -26:19:32.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27338_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 27338_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:12:16.11 -28:25:00.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07372_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 07372_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:45:46.33 -30:02:30.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 73423_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:25:34.66 -23:26:54.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59377_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 59377_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:03:54.74 -24:43:34.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77383_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 77383_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:08:43.69 -23:41:08.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24054_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 24054_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28288_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 28288_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49830_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 49830_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:03:20.96 -25:51:53.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14702_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 14702_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:24:39.78 -29:42:12.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16992_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 16992_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:11:02.10 -29:24:53.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77140_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 77140_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:06:06.39 -23:36:23.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81524_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 81524_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:48:26.56 -23:50:03.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28857_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 28857_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:35:52.17 -28:12:48.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61209_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
Preparing report for the candidate 61209_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27268_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 27268_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:46:12.73 -28:03:42.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10177_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 10177_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:52:12.67 -29:53:12.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19168_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 19168_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:02:39.66 -29:08:07.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 43915_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:34.74 -26:17:23.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02768_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 02768_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:19:32.64 -30:54:14.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46946_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 46946_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:58:51.78 -26:06:45.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84434_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 84434_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:41:36.12 -24:28:05.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 35726_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:54:30.20 -27:20:19.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58372_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 58372_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:58:35.13 -24:49:54.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25979_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 25979_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:44:59.95 -28:30:33.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54623_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 54623_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:54:39.58 -25:14:38.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 67349_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:00:20.47 -22:37:21.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45501_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 45501_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:55:30.22 -26:15:57.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69736_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 69736_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:53:54.08 -24:32:00.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17193_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 17193_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:56:53.50 -29:12:43.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48797_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 48797_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:50:59.15 -25:45:03.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53620_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 53620_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:53:37.18 -25:19:36.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62014_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 62014_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 15:57:40.52 -20:59:00.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60722_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009
The candidate 60722_fd_Sco-02-Q1b1x1_2026-04-20_05-11-59_20.00sec_-4.90C_LIGHTs_0009 did not pass the final checks
**** FOUND 16:07:24.64 -20:52:13.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 12s
make_report_in_HTML.sh TOTAL: 581s
Prepared the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:23:35.42 -26:31:37.7
16:52:09.48 -28:12:42.5
16:53:14.38 -29:31:09.5
16:50:23.00 -28:32:20.9
16:43:06.15 -21:41:24.0
16:44:19.94 -26:19:30.5
16:24:16.94 -31:10:22.5
16:46:15.66 -29:09:41.6
16:43:46.69 -25:13:32.6
16:13:23.98 -21:58:10.0
16:51:43.72 -23:54:10.9
16:48:52.24 -28:26:08.4
16:46:54.24 -30:07:53.4
16:45:20.68 -26:54:43.3
16:49:51.34 -24:26:52.8
16:43:43.36 -30:45:03.1
16:20:04.22 -31:00:51.6
16:09:27.83 -30:56:35.4
15:50:02.62 -30:25:52.7
16:44:13.73 -30:41:33.1
16:23:18.46 -30:38:28.6
16:39:14.70 -30:24:22.5
16:14:22.01 -28:01:16.5
16:08:03.37 -25:33:07.6
16:08:18.50 -27:17:11.6
15:43:39.68 -28:24:04.2
15:43:36.88 -29:14:38.9
15:43:18.82 -28:16:54.0
15:45:50.62 -27:52:55.7
16:44:40.05 -30:23:22.3
16:01:33.03 -29:05:56.0
15:52:10.68 -25:55:30.2
15:46:47.40 -29:27:31.4
15:59:51.81 -28:08:51.3
15:51:36.48 -28:19:08.1
16:30:23.67 -30:05:02.0
15:55:22.15 -22:07:22.9
15:46:51.53 -28:21:55.7
15:46:19.36 -27:13:15.2
16:22:21.71 -30:51:17.2
16:10:31.99 -29:01:39.8
15:46:09.94 -24:18:31.5
16:03:21.30 -28:45:09.6
15:52:04.24 -21:11:00.5
15:59:18.42 -28:49:45.9
15:59:07.34 -21:50:41.4
16:03:55.67 -24:32:35.8
15:50:08.82 -23:33:23.1
16:02:36.33 -26:44:13.5
15:54:55.13 -26:34:47.9
15:46:13.78 -28:27:49.6
15:51:36.80 -28:19:11.0
15:44:38.04 -27:40:12.7
15:46:51.57 -26:16:15.4
16:09:46.74 -30:23:54.2
16:41:21.66 -30:36:21.7
16:40:45.38 -31:05:31.7
15:55:04.93 -29:58:22.7
16:21:10.73 -27:53:04.1
15:45:40.81 -26:35:12.7
15:53:46.85 -28:58:16.6
16:40:44.36 -30:29:38.4
15:49:57.78 -21:47:19.5
15:46:39.49 -24:59:09.5
16:35:57.38 -26:49:34.8
16:44:00.37 -25:29:57.9
15:51:52.12 -28:56:49.5
15:48:59.83 -30:17:18.3
16:37:05.09 -29:53:35.5
15:48:12.91 -27:13:12.5
16:53:10.74 -29:07:44.7
15:48:16.61 -28:18:27.1
15:48:14.67 -26:10:25.1
15:50:29.06 -20:40:25.1
16:03:54.02 -27:40:31.8
15:44:14.24 -29:32:00.7
15:49:55.52 -29:04:17.7
16:45:24.16 -28:31:44.6
15:47:55.16 -29:38:04.8
16:49:58.85 -30:38:19.6
15:43:30.18 -28:25:13.8
15:45:39.43 -27:45:33.0
15:46:10.98 -27:36:48.3
15:59:38.31 -21:10:43.1
15:43:54.30 -29:41:30.0
16:07:33.66 -29:41:13.3
15:45:42.96 -25:44:31.8
16:49:29.05 -31:04:15.9
16:50:44.80 -30:18:17.4
15:45:30.81 -27:58:17.5
16:53:22.02 -29:43:16.9
15:53:45.96 -27:16:25.9
15:46:55.93 -22:16:18.4
16:49:37.84 -30:24:59.8
15:43:58.25 -29:32:18.2
15:45:05.59 -30:13:20.0
16:46:13.27 -29:46:18.6
16:49:06.33 -22:48:55.9
16:49:18.35 -28:02:13.2
16:53:25.16 -29:56:29.4
15:44:41.25 -27:55:43.5
16:47:08.97 -31:11:01.8
16:52:33.24 -29:17:25.9
15:45:01.24 -30:08:11.0
16:41:41.62 -29:26:40.2
16:46:43.92 -24:52:08.8
16:29:18.30 -30:20:41.8
15:49:28.48 -20:31:27.2
16:53:05.25 -30:38:15.9
16:45:45.70 -28:50:38.2
16:19:48.98 -22:17:37.1
16:50:46.59 -30:07:55.5
16:19:04.53 -29:54:16.3
16:41:46.00 -21:12:43.8
16:26:59.80 -27:55:10.7
16:47:27.34 -22:08:47.5
16:45:26.17 -30:58:52.3
16:47:45.23 -27:37:40.7
16:51:19.97 -28:39:28.8
16:48:33.49 -25:50:33.8
16:01:07.77 -27:36:07.1
16:51:47.43 -25:38:14.9
16:33:54.17 -28:12:42.4
16:48:00.38 -28:53:32.6
16:52:48.67 -30:36:24.1
16:49:04.81 -28:14:44.5
16:52:44.92 -26:36:39.6
16:47:25.37 -23:58:16.2
15:53:39.16 -27:07:15.0
16:52:23.89 -23:34:13.5
16:52:08.21 -28:08:52.9
16:52:43.50 -24:26:08.0
16:48:22.23 -26:05:37.2
16:12:51.65 -24:45:29.1
16:47:04.94 -25:48:42.3
15:51:45.03 -24:49:27.3
16:11:29.68 -27:12:38.9
16:41:02.21 -29:19:48.1
16:44:02.37 -26:58:20.4
16:42:31.49 -24:38:08.6
16:51:35.56 -29:55:38.1
16:51:29.02 -29:05:27.9
16:41:59.41 -29:44:48.6
16:50:53.23 -23:28:24.0
16:47:53.49 -29:45:24.3
16:49:07.29 -23:11:32.6
16:53:16.51 -28:44:26.9
16:52:34.37 -30:39:27.7
16:53:43.51 -23:13:04.7
16:48:12.82 -23:20:44.7
16:43:51.55 -26:43:04.5
16:48:36.21 -26:02:22.2
16:44:28.32 -29:55:23.4
16:53:00.82 -27:34:28.6
15:51:50.92 -20:56:52.8
16:51:59.48 -21:28:54.4
16:44:17.45 -22:06:53.4
16:21:15.19 -29:00:33.2
16:19:33.16 -21:55:41.3
16:48:58.07 -26:13:47.0
15:57:29.88 -20:50:56.5
16:47:04.30 -25:48:40.7
16:46:11.08 -29:29:15.5
16:51:37.18 -24:47:58.2
16:53:01.49 -30:12:02.9
16:52:00.63 -28:00:49.6
16:49:47.56 -27:33:22.5
16:48:13.35 -24:15:53.4
16:19:12.61 -31:06:40.6
16:52:50.90 -29:00:02.0
16:47:53.69 -31:06:09.7
16:26:48.67 -30:35:38.1
16:44:25.82 -27:57:21.3
16:02:56.42 -30:30:59.4
15:51:27.32 -29:11:13.7
16:02:18.75 -20:39:24.8
16:53:03.64 -28:34:45.0
16:42:57.18 -24:47:27.5
15:57:17.70 -20:34:30.5
16:53:21.52 -29:12:39.2
16:51:46.35 -22:28:38.8
16:41:01.72 -29:19:58.1
16:04:25.55 -21:17:17.6
16:49:25.33 -23:33:25.8
16:47:48.94 -27:15:59.9
15:52:57.36 -26:39:27.4
16:37:29.29 -28:31:54.1
16:47:50.31 -29:09:57.8
16:40:41.55 -28:09:48.4
16:46:02.78 -29:37:25.3
16:52:06.26 -21:46:38.3
16:29:17.72 -30:22:22.9
16:23:57.83 -26:39:21.0
15:51:26.26 -26:10:27.4
16:03:29.09 -25:11:28.7
16:47:27.71 -22:27:42.3
16:44:27.44 -29:55:53.7
16:48:15.00 -22:44:24.9
16:16:10.57 -22:34:12.8
16:11:13.63 -22:57:38.0
16:02:15.55 -23:17:11.3
16:37:29.24 -29:28:54.0
16:27:10.14 -29:24:36.9
16:48:31.85 -28:45:18.7
16:08:00.35 -22:45:34.6
16:23:38.71 -25:46:45.4
15:52:37.19 -27:42:54.6
16:11:06.53 -23:21:07.8
16:45:33.93 -29:20:03.5
16:32:45.99 -27:17:48.7
16:48:41.02 -27:25:00.6
15:54:49.55 -30:25:53.0
16:19:43.95 -28:59:27.8
16:49:20.61 -22:34:12.0
16:23:42.53 -29:01:37.0
16:09:12.12 -23:36:00.1
16:42:45.43 -28:47:47.2
16:52:19.47 -22:04:15.8
16:03:25.55 -30:38:06.5
16:31:27.00 -31:12:46.9
15:54:45.72 -25:23:15.7
16:39:12.44 -23:29:12.9
16:40:00.12 -30:19:25.5
16:35:15.67 -31:07:49.7
16:04:35.93 -29:43:24.1
16:05:44.05 -25:18:34.0
16:03:51.42 -27:36:55.3
16:03:53.62 -24:58:59.5
15:53:31.90 -29:42:45.0
15:46:29.73 -26:29:16.5
16:04:21.32 -27:20:11.9
16:06:24.31 -26:15:19.6
16:36:31.83 -27:21:36.3
16:05:19.52 -30:42:03.9
16:46:39.40 -23:23:17.9
15:50:57.58 -26:09:25.2
15:50:13.62 -29:38:25.4
16:53:21.09 -29:48:56.1
16:47:45.07 -29:51:38.6
16:23:18.03 -29:53:50.2
16:46:51.02 -29:48:14.8
16:48:47.85 -29:45:44.8
16:50:11.89 -29:43:30.3
16:53:13.99 -29:40:47.8
16:46:02.04 -29:43:13.2
15:57:02.17 -28:56:19.7
16:52:04.59 -28:59:32.4
16:02:06.58 -28:54:33.4
16:42:39.40 -28:55:44.5
16:08:06.20 -28:47:29.5
16:12:47.37 -28:44:09.2
16:52:39.12 -28:36:07.9
16:50:22.42 -28:32:21.8
16:45:41.11 -28:23:20.4
16:45:13.95 -28:20:12.3
16:48:35.39 -28:15:35.4
16:18:31.82 -28:19:39.4
16:47:54.33 -28:09:22.2
16:07:01.00 -28:01:36.6
16:53:26.81 -27:55:55.9
15:52:50.84 -27:25:23.1
16:49:08.32 -27:24:44.4
15:58:10.99 -26:58:07.0
16:47:10.20 -26:35:35.8
16:48:58.04 -26:27:09.3
16:41:59.22 -26:21:43.1
16:02:53.02 -26:03:07.8
16:52:26.93 -25:54:30.3
16:43:52.90 -25:04:30.3
16:10:26.11 -20:50:39.5
15:52:57.91 -20:46:46.8
16:17:37.50 -21:09:37.2
16:42:12.04 -22:42:16.6
15:46:46.05 -24:30:52.3
15:55:38.35 -22:10:59.2
16:27:12.50 -26:01:17.7
16:37:47.70 -27:20:57.3
16:08:06.80 -30:14:48.9
########### Completed Sco-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
16:52:09.48 -28:12:42.5
16:53:14.38 -29:31:09.5
16:50:23.00 -28:32:20.9
16:43:06.15 -21:41:24.0
16:44:19.94 -26:19:30.5
16:24:16.94 -31:10:22.5
16:46:15.66 -29:09:41.6
16:43:46.69 -25:13:32.6
16:13:23.98 -21:58:10.0
16:51:43.72 -23:54:10.9
16:48:52.24 -28:26:08.4
16:46:54.24 -30:07:53.4
16:45:20.68 -26:54:43.3
16:49:51.34 -24:26:52.8
16:43:43.36 -30:45:03.1
16:23:35.42 -26:31:37.7
16:14:22.01 -28:01:16.5
16:08:03.37 -25:33:07.6
16:08:18.50 -27:17:11.6
15:43:39.68 -28:24:04.2
15:43:36.88 -29:14:38.9
15:43:18.82 -28:16:54.0
15:45:50.62 -27:52:55.7
16:44:40.05 -30:23:22.3
16:01:33.03 -29:05:56.0
15:52:10.68 -25:55:30.2
15:46:47.40 -29:27:31.4
15:59:51.81 -28:08:51.3
15:51:36.48 -28:19:08.1
16:30:23.67 -30:05:02.0
15:55:22.15 -22:07:22.9
15:46:51.53 -28:21:55.7
15:46:19.36 -27:13:15.2
16:22:21.71 -30:51:17.2
16:10:31.99 -29:01:39.8
15:46:09.94 -24:18:31.5
16:03:21.30 -28:45:09.6
15:52:04.24 -21:11:00.5
15:59:18.42 -28:49:45.9
15:59:07.34 -21:50:41.4
16:03:55.67 -24:32:35.8
15:50:08.82 -23:33:23.1
16:02:36.33 -26:44:13.5
15:54:55.13 -26:34:47.9
15:46:13.78 -28:27:49.6
15:51:36.80 -28:19:11.0
15:44:38.04 -27:40:12.7
15:46:51.57 -26:16:15.4
16:09:46.74 -30:23:54.2
16:41:21.66 -30:36:21.7
16:40:45.38 -31:05:31.7
15:55:04.93 -29:58:22.7
16:21:10.73 -27:53:04.1
15:45:40.81 -26:35:12.7
15:53:46.85 -28:58:16.6
16:40:44.36 -30:29:38.4
15:49:57.78 -21:47:19.5
15:46:39.49 -24:59:09.5
16:35:57.38 -26:49:34.8
16:44:00.37 -25:29:57.9
15:51:52.12 -28:56:49.5
15:48:59.83 -30:17:18.3
16:37:05.09 -29:53:35.5
15:48:12.91 -27:13:12.5
16:53:10.74 -29:07:44.7
15:48:16.61 -28:18:27.1
15:48:14.67 -26:10:25.1
15:50:29.06 -20:40:25.1
16:03:54.02 -27:40:31.8
15:44:14.24 -29:32:00.7
15:49:55.52 -29:04:17.7
16:45:24.16 -28:31:44.6
15:47:55.16 -29:38:04.8
16:49:58.85 -30:38:19.6
15:43:30.18 -28:25:13.8
15:45:39.43 -27:45:33.0
15:46:10.98 -27:36:48.3
15:59:38.31 -21:10:43.1
15:43:54.30 -29:41:30.0
16:07:33.66 -29:41:13.3
15:45:42.96 -25:44:31.8
16:49:29.05 -31:04:15.9
16:50:44.80 -30:18:17.4
15:45:30.81 -27:58:17.5
16:53:22.02 -29:43:16.9
15:53:45.96 -27:16:25.9
15:46:55.93 -22:16:18.4
16:49:37.84 -30:24:59.8
15:43:58.25 -29:32:18.2
15:45:05.59 -30:13:20.0
16:46:13.27 -29:46:18.6
16:49:06.33 -22:48:55.9
16:49:18.35 -28:02:13.2
16:53:25.16 -29:56:29.4
15:44:41.25 -27:55:43.5
16:47:08.97 -31:11:01.8
16:52:33.24 -29:17:25.9
15:45:01.24 -30:08:11.0
16:41:41.62 -29:26:40.2
16:46:43.92 -24:52:08.8
16:29:18.30 -30:20:41.8
15:49:28.48 -20:31:27.2
16:53:05.25 -30:38:15.9
16:45:45.70 -28:50:38.2
16:19:48.98 -22:17:37.1
16:50:46.59 -30:07:55.5
16:19:04.53 -29:54:16.3
16:41:46.00 -21:12:43.8
16:26:59.80 -27:55:10.7
16:47:27.34 -22:08:47.5
16:45:26.17 -30:58:52.3
16:47:45.23 -27:37:40.7
16:51:19.97 -28:39:28.8
16:48:33.49 -25:50:33.8
16:01:07.77 -27:36:07.1
16:51:47.43 -25:38:14.9
16:33:54.17 -28:12:42.4
16:48:00.38 -28:53:32.6
16:52:48.67 -30:36:24.1
16:49:04.81 -28:14:44.5
16:52:44.92 -26:36:39.6
16:47:25.37 -23:58:16.2
15:53:39.16 -27:07:15.0
16:52:23.89 -23:34:13.5
16:52:08.21 -28:08:52.9
16:52:43.50 -24:26:08.0
16:48:22.23 -26:05:37.2
16:12:51.65 -24:45:29.1
16:47:04.94 -25:48:42.3
15:51:45.03 -24:49:27.3
16:11:29.68 -27:12:38.9
16:41:02.21 -29:19:48.1
16:44:02.37 -26:58:20.4
16:42:31.49 -24:38:08.6
16:51:35.56 -29:55:38.1
16:51:29.02 -29:05:27.9
16:41:59.41 -29:44:48.6
16:50:53.23 -23:28:24.0
16:47:53.49 -29:45:24.3
16:49:07.29 -23:11:32.6
16:53:16.51 -28:44:26.9
16:52:34.37 -30:39:27.7
16:53:43.51 -23:13:04.7
16:48:12.82 -23:20:44.7
16:43:51.55 -26:43:04.5
16:48:36.21 -26:02:22.2
16:44:28.32 -29:55:23.4
16:53:00.82 -27:34:28.6
15:51:50.92 -20:56:52.8
16:51:59.48 -21:28:54.4
16:44:17.45 -22:06:53.4
16:21:15.19 -29:00:33.2
16:19:33.16 -21:55:41.3
16:48:58.07 -26:13:47.0
15:57:29.88 -20:50:56.5
16:47:04.30 -25:48:40.7
16:46:11.08 -29:29:15.5
16:51:37.18 -24:47:58.2
16:53:01.49 -30:12:02.9
16:52:00.63 -28:00:49.6
16:49:47.56 -27:33:22.5
16:48:13.35 -24:15:53.4
16:19:12.61 -31:06:40.6
16:52:50.90 -29:00:02.0
16:47:53.69 -31:06:09.7
16:26:48.67 -30:35:38.1
16:44:25.82 -27:57:21.3
16:02:56.42 -30:30:59.4
15:51:27.32 -29:11:13.7
16:02:18.75 -20:39:24.8
16:53:03.64 -28:34:45.0
16:42:57.18 -24:47:27.5
15:57:17.70 -20:34:30.5
16:53:21.52 -29:12:39.2
16:51:46.35 -22:28:38.8
16:41:01.72 -29:19:58.1
16:04:25.55 -21:17:17.6
16:49:25.33 -23:33:25.8
16:47:48.94 -27:15:59.9
15:52:57.36 -26:39:27.4
16:37:29.29 -28:31:54.1
16:47:50.31 -29:09:57.8
16:40:41.55 -28:09:48.4
16:46:02.78 -29:37:25.3
16:52:06.26 -21:46:38.3
16:29:17.72 -30:22:22.9
16:23:57.83 -26:39:21.0
15:51:26.26 -26:10:27.4
16:03:29.09 -25:11:28.7
16:47:27.71 -22:27:42.3
16:44:27.44 -29:55:53.7
16:48:15.00 -22:44:24.9
16:16:10.57 -22:34:12.8
16:11:13.63 -22:57:38.0
16:02:15.55 -23:17:11.3
16:37:29.24 -29:28:54.0
16:27:10.14 -29:24:36.9
16:48:31.85 -28:45:18.7
16:08:00.35 -22:45:34.6
16:23:38.71 -25:46:45.4
15:52:37.19 -27:42:54.6
16:11:06.53 -23:21:07.8
16:45:33.93 -29:20:03.5
16:32:45.99 -27:17:48.7
16:48:41.02 -27:25:00.6
15:54:49.55 -30:25:53.0
16:19:43.95 -28:59:27.8
16:49:20.61 -22:34:12.0
16:23:42.53 -29:01:37.0
16:09:12.12 -23:36:00.1
16:42:45.43 -28:47:47.2
16:52:19.47 -22:04:15.8
16:03:25.55 -30:38:06.5
16:31:27.00 -31:12:46.9
15:54:45.72 -25:23:15.7
16:39:12.44 -23:29:12.9
16:40:00.12 -30:19:25.5
16:35:15.67 -31:07:49.7
16:04:35.93 -29:43:24.1
16:05:44.05 -25:18:34.0
16:03:51.42 -27:36:55.3
16:03:53.62 -24:58:59.5
15:53:31.90 -29:42:45.0
15:46:29.73 -26:29:16.5
16:04:21.32 -27:20:11.9
16:06:24.31 -26:15:19.6
16:36:31.83 -27:21:36.3
16:05:19.52 -30:42:03.9
16:46:39.40 -23:23:17.9
15:50:57.58 -26:09:25.2
16:08:06.80 -30:14:48.9
15:46:46.05 -24:30:52.3
16:23:18.03 -29:53:50.2
16:53:26.81 -27:55:55.9
16:39:14.70 -30:24:22.5
16:02:06.58 -28:54:33.4
15:55:38.35 -22:10:59.2
16:46:51.02 -29:48:14.8
16:47:45.07 -29:51:38.6
16:52:39.12 -28:36:07.9
16:02:53.02 -26:03:07.8
16:12:47.37 -28:44:09.2
16:41:59.22 -26:21:43.1
16:09:27.83 -30:56:35.4
16:45:13.95 -28:20:12.3
16:48:47.85 -29:45:44.8
16:10:26.11 -20:50:39.5
16:50:22.42 -28:32:21.8
16:53:13.99 -29:40:47.8
16:23:18.46 -30:38:28.6
15:52:50.84 -27:25:23.1
16:17:37.50 -21:09:37.2
16:07:01.00 -28:01:36.6
16:47:54.33 -28:09:22.2
16:49:08.32 -27:24:44.4
15:57:02.17 -28:56:19.7
16:46:02.04 -29:43:13.2
16:20:04.22 -31:00:51.6
16:47:10.20 -26:35:35.8
16:53:21.09 -29:48:56.1
16:52:26.93 -25:54:30.3
16:37:47.70 -27:20:57.3
16:27:12.50 -26:01:17.7
16:18:31.82 -28:19:39.4
15:50:13.62 -29:38:25.4
15:58:10.99 -26:58:07.0
16:50:11.89 -29:43:30.3
16:52:04.59 -28:59:32.4
16:48:58.04 -26:27:09.3
16:44:13.73 -30:41:33.1
16:43:52.90 -25:04:30.3
16:42:39.40 -28:55:44.5
16:42:12.04 -22:42:16.6
16:48:35.39 -28:15:35.4
15:50:02.62 -30:25:52.7
16:08:06.20 -28:47:29.5
16:45:41.11 -28:23:20.4
15:52:57.91 -20:46:46.8
###################################################################################
16:52:09.48 -28:12:42.5 -- not an asteroid (will add it to exclusion list)
16:53:14.38 -29:31:09.5 -- not an asteroid (will add it to exclusion list)
16:50:23.00 -28:32:20.9 -- not an asteroid (will add it to exclusion list)
16:43:06.15 -21:41:24.0 -- not an asteroid (will add it to exclusion list)
16:44:19.94 -26:19:30.5 -- not an asteroid (will add it to exclusion list)
16:24:16.94 -31:10:22.5 -- not an asteroid (will add it to exclusion list)
16:46:15.66 -29:09:41.6 -- not an asteroid (will add it to exclusion list)
16:43:46.69 -25:13:32.6 -- not an asteroid (will add it to exclusion list)
16:13:23.98 -21:58:10.0 -- not an asteroid (will add it to exclusion list)
16:51:43.72 -23:54:10.9 -- not an asteroid (will add it to exclusion list)
16:48:52.24 -28:26:08.4 -- not an asteroid (will add it to exclusion list)
16:46:54.24 -30:07:53.4 -- asteroid (will NOT add it to exclusion list)
16:45:20.68 -26:54:43.3 -- asteroid (will NOT add it to exclusion list)
16:49:51.34 -24:26:52.8 -- asteroid (will NOT add it to exclusion list)
16:43:43.36 -30:45:03.1 -- not an asteroid (will add it to exclusion list)
16:23:35.42 -26:31:37.7 -- not an asteroid (will add it to exclusion list)
16:14:22.01 -28:01:16.5 -- not an asteroid (will add it to exclusion list)
16:08:03.37 -25:33:07.6 -- not an asteroid (will add it to exclusion list)
16:08:18.50 -27:17:11.6 -- not an asteroid (will add it to exclusion list)
15:43:39.68 -28:24:04.2 -- not an asteroid (will add it to exclusion list)
15:43:36.88 -29:14:38.9 -- not an asteroid (will add it to exclusion list)
15:43:18.82 -28:16:54.0 -- not an asteroid (will add it to exclusion list)
15:45:50.62 -27:52:55.7 -- not an asteroid (will add it to exclusion list)
16:44:40.05 -30:23:22.3 -- not an asteroid (will add it to exclusion list)
16:01:33.03 -29:05:56.0 -- asteroid (will NOT add it to exclusion list)
15:52:10.68 -25:55:30.2 -- not an asteroid (will add it to exclusion list)
15:46:47.40 -29:27:31.4 -- not an asteroid (will add it to exclusion list)
15:59:51.81 -28:08:51.3 -- asteroid (will NOT add it to exclusion list)
15:51:36.48 -28:19:08.1 -- not an asteroid (will add it to exclusion list)
16:30:23.67 -30:05:02.0 -- not an asteroid (will add it to exclusion list)
15:55:22.15 -22:07:22.9 -- not an asteroid (will add it to exclusion list)
15:46:51.53 -28:21:55.7 -- not an asteroid (will add it to exclusion list)
15:46:19.36 -27:13:15.2 -- not an asteroid (will add it to exclusion list)
16:22:21.71 -30:51:17.2 -- not an asteroid (will add it to exclusion list)
16:10:31.99 -29:01:39.8 -- not an asteroid (will add it to exclusion list)
15:46:09.94 -24:18:31.5 -- not an asteroid (will add it to exclusion list)
16:03:21.30 -28:45:09.6 -- not an asteroid (will add it to exclusion list)
15:52:04.24 -21:11:00.5 -- not an asteroid (will add it to exclusion list)
15:59:18.42 -28:49:45.9 -- not an asteroid (will add it to exclusion list)
15:59:07.34 -21:50:41.4 -- not an asteroid (will add it to exclusion list)
16:03:55.67 -24:32:35.8 -- not an asteroid (will add it to exclusion list)
15:50:08.82 -23:33:23.1 -- not an asteroid (will add it to exclusion list)
16:02:36.33 -26:44:13.5 -- not an asteroid (will add it to exclusion list)
15:54:55.13 -26:34:47.9 -- not an asteroid (will add it to exclusion list)
15:46:13.78 -28:27:49.6 -- not an asteroid (will add it to exclusion list)
15:51:36.80 -28:19:11.0 -- not an asteroid (will add it to exclusion list)
15:44:38.04 -27:40:12.7 -- not an asteroid (will add it to exclusion list)
15:46:51.57 -26:16:15.4 -- not an asteroid (will add it to exclusion list)
16:09:46.74 -30:23:54.2 -- not an asteroid (will add it to exclusion list)
16:41:21.66 -30:36:21.7 -- not an asteroid (will add it to exclusion list)
16:40:45.38 -31:05:31.7 -- not an asteroid (will add it to exclusion list)
15:55:04.93 -29:58:22.7 -- not an asteroid (will add it to exclusion list)
16:21:10.73 -27:53:04.1 -- not an asteroid (will add it to exclusion list)
15:45:40.81 -26:35:12.7 -- not an asteroid (will add it to exclusion list)
15:53:46.85 -28:58:16.6 -- asteroid (will NOT add it to exclusion list)
16:40:44.36 -30:29:38.4 -- not an asteroid (will add it to exclusion list)
15:49:57.78 -21:47:19.5 -- not an asteroid (will add it to exclusion list)
15:46:39.49 -24:59:09.5 -- not an asteroid (will add it to exclusion list)
16:35:57.38 -26:49:34.8 -- not an asteroid (will add it to exclusion list)
16:44:00.37 -25:29:57.9 -- not an asteroid (will add it to exclusion list)
15:51:52.12 -28:56:49.5 -- not an asteroid (will add it to exclusion list)
15:48:59.83 -30:17:18.3 -- not an asteroid (will add it to exclusion list)
16:37:05.09 -29:53:35.5 -- not an asteroid (will add it to exclusion list)
15:48:12.91 -27:13:12.5 -- not an asteroid (will add it to exclusion list)
16:53:10.74 -29:07:44.7 -- not an asteroid (will add it to exclusion list)
15:48:16.61 -28:18:27.1 -- not an asteroid (will add it to exclusion list)
15:48:14.67 -26:10:25.1 -- not an asteroid (will add it to exclusion list)
15:50:29.06 -20:40:25.1 -- not an asteroid (will add it to exclusion list)
16:03:54.02 -27:40:31.8 -- not an asteroid (will add it to exclusion list)
15:44:14.24 -29:32:00.7 -- not an asteroid (will add it to exclusion list)
15:49:55.52 -29:04:17.7 -- not an asteroid (will add it to exclusion list)
16:45:24.16 -28:31:44.6 -- not an asteroid (will add it to exclusion list)
15:47:55.16 -29:38:04.8 -- not an asteroid (will add it to exclusion list)
16:49:58.85 -30:38:19.6 -- not an asteroid (will add it to exclusion list)
15:43:30.18 -28:25:13.8 -- not an asteroid (will add it to exclusion list)
15:45:39.43 -27:45:33.0 -- not an asteroid (will add it to exclusion list)
15:46:10.98 -27:36:48.3 -- not an asteroid (will add it to exclusion list)
15:59:38.31 -21:10:43.1 -- not an asteroid (will add it to exclusion list)
15:43:54.30 -29:41:30.0 -- not an asteroid (will add it to exclusion list)
16:07:33.66 -29:41:13.3 -- not an asteroid (will add it to exclusion list)
15:45:42.96 -25:44:31.8 -- not an asteroid (will add it to exclusion list)
16:49:29.05 -31:04:15.9 -- not an asteroid (will add it to exclusion list)
16:50:44.80 -30:18:17.4 -- not an asteroid (will add it to exclusion list)
15:45:30.81 -27:58:17.5 -- not an asteroid (will add it to exclusion list)
16:53:22.02 -29:43:16.9 -- not an asteroid (will add it to exclusion list)
15:53:45.96 -27:16:25.9 -- not an asteroid (will add it to exclusion list)
15:46:55.93 -22:16:18.4 -- not an asteroid (will add it to exclusion list)
16:49:37.84 -30:24:59.8 -- not an asteroid (will add it to exclusion list)
15:43:58.25 -29:32:18.2 -- not an asteroid (will add it to exclusion list)
15:45:05.59 -30:13:20.0 -- not an asteroid (will add it to exclusion list)
16:46:13.27 -29:46:18.6 -- not an asteroid (will add it to exclusion list)
16:49:06.33 -22:48:55.9 -- not an asteroid (will add it to exclusion list)
16:49:18.35 -28:02:13.2 -- not an asteroid (will add it to exclusion list)
16:53:25.16 -29:56:29.4 -- not an asteroid (will add it to exclusion list)
15:44:41.25 -27:55:43.5 -- not an asteroid (will add it to exclusion list)
16:47:08.97 -31:11:01.8 -- not an asteroid (will add it to exclusion list)
16:52:33.24 -29:17:25.9 -- not an asteroid (will add it to exclusion list)
15:45:01.24 -30:08:11.0 -- not an asteroid (will add it to exclusion list)
16:41:41.62 -29:26:40.2 -- not an asteroid (will add it to exclusion list)
16:46:43.92 -24:52:08.8 -- not an asteroid (will add it to exclusion list)
16:29:18.30 -30:20:41.8 -- not an asteroid (will add it to exclusion list)
15:49:28.48 -20:31:27.2 -- not an asteroid (will add it to exclusion list)
16:53:05.25 -30:38:15.9 -- not an asteroid (will add it to exclusion list)
16:45:45.70 -28:50:38.2 -- not an asteroid (will add it to exclusion list)
16:19:48.98 -22:17:37.1 -- not an asteroid (will add it to exclusion list)
16:50:46.59 -30:07:55.5 -- not an asteroid (will add it to exclusion list)
16:19:04.53 -29:54:16.3 -- not an asteroid (will add it to exclusion list)
16:41:46.00 -21:12:43.8 -- not an asteroid (will add it to exclusion list)
16:26:59.80 -27:55:10.7 -- not an asteroid (will add it to exclusion list)
16:47:27.34 -22:08:47.5 -- not an asteroid (will add it to exclusion list)
16:45:26.17 -30:58:52.3 -- not an asteroid (will add it to exclusion list)
16:47:45.23 -27:37:40.7 -- not an asteroid (will add it to exclusion list)
16:51:19.97 -28:39:28.8 -- not an asteroid (will add it to exclusion list)
16:48:33.49 -25:50:33.8 -- not an asteroid (will add it to exclusion list)
16:01:07.77 -27:36:07.1 -- not an asteroid (will add it to exclusion list)
16:51:47.43 -25:38:14.9 -- not an asteroid (will add it to exclusion list)
16:33:54.17 -28:12:42.4 -- not an asteroid (will add it to exclusion list)
16:48:00.38 -28:53:32.6 -- not an asteroid (will add it to exclusion list)
16:52:48.67 -30:36:24.1 -- not an asteroid (will add it to exclusion list)
16:49:04.81 -28:14:44.5 -- not an asteroid (will add it to exclusion list)
16:52:44.92 -26:36:39.6 -- not an asteroid (will add it to exclusion list)
16:47:25.37 -23:58:16.2 -- not an asteroid (will add it to exclusion list)
15:53:39.16 -27:07:15.0 -- not an asteroid (will add it to exclusion list)
16:52:23.89 -23:34:13.5 -- not an asteroid (will add it to exclusion list)
16:52:08.21 -28:08:52.9 -- not an asteroid (will add it to exclusion list)
16:52:43.50 -24:26:08.0 -- not an asteroid (will add it to exclusion list)
16:48:22.23 -26:05:37.2 -- not an asteroid (will add it to exclusion list)
16:12:51.65 -24:45:29.1 -- not an asteroid (will add it to exclusion list)
16:47:04.94 -25:48:42.3 -- not an asteroid (will add it to exclusion list)
15:51:45.03 -24:49:27.3 -- not an asteroid (will add it to exclusion list)
16:11:29.68 -27:12:38.9 -- asteroid (will NOT add it to exclusion list)
16:41:02.21 -29:19:48.1 -- not an asteroid (will add it to exclusion list)
16:44:02.37 -26:58:20.4 -- not an asteroid (will add it to exclusion list)
16:42:31.49 -24:38:08.6 -- not an asteroid (will add it to exclusion list)
16:51:35.56 -29:55:38.1 -- not an asteroid (will add it to exclusion list)
16:51:29.02 -29:05:27.9 -- not an asteroid (will add it to exclusion list)
16:41:59.41 -29:44:48.6 -- not an asteroid (will add it to exclusion list)
16:50:53.23 -23:28:24.0 -- not an asteroid (will add it to exclusion list)
16:47:53.49 -29:45:24.3 -- not an asteroid (will add it to exclusion list)
16:49:07.29 -23:11:32.6 -- not an asteroid (will add it to exclusion list)
16:53:16.51 -28:44:26.9 -- not an asteroid (will add it to exclusion list)
16:52:34.37 -30:39:27.7 -- not an asteroid (will add it to exclusion list)
16:53:43.51 -23:13:04.7 -- not an asteroid (will add it to exclusion list)
16:48:12.82 -23:20:44.7 -- not an asteroid (will add it to exclusion list)
16:43:51.55 -26:43:04.5 -- not an asteroid (will add it to exclusion list)
16:48:36.21 -26:02:22.2 -- not an asteroid (will add it to exclusion list)
16:44:28.32 -29:55:23.4 -- not an asteroid (will add it to exclusion list)
16:53:00.82 -27:34:28.6 -- not an asteroid (will add it to exclusion list)
15:51:50.92 -20:56:52.8 -- not an asteroid (will add it to exclusion list)
16:51:59.48 -21:28:54.4 -- not an asteroid (will add it to exclusion list)
16:44:17.45 -22:06:53.4 -- not an asteroid (will add it to exclusion list)
16:21:15.19 -29:00:33.2 -- not an asteroid (will add it to exclusion list)
16:19:33.16 -21:55:41.3 -- not an asteroid (will add it to exclusion list)
16:48:58.07 -26:13:47.0 -- not an asteroid (will add it to exclusion list)
15:57:29.88 -20:50:56.5 -- not an asteroid (will add it to exclusion list)
16:47:04.30 -25:48:40.7 -- not an asteroid (will add it to exclusion list)
16:46:11.08 -29:29:15.5 -- not an asteroid (will add it to exclusion list)
16:51:37.18 -24:47:58.2 -- not an asteroid (will add it to exclusion list)
16:53:01.49 -30:12:02.9 -- not an asteroid (will add it to exclusion list)
16:52:00.63 -28:00:49.6 -- not an asteroid (will add it to exclusion list)
16:49:47.56 -27:33:22.5 -- not an asteroid (will add it to exclusion list)
16:48:13.35 -24:15:53.4 -- asteroid (will NOT add it to exclusion list)
16:19:12.61 -31:06:40.6 -- not an asteroid (will add it to exclusion list)
16:52:50.90 -29:00:02.0 -- not an asteroid (will add it to exclusion list)
16:47:53.69 -31:06:09.7 -- not an asteroid (will add it to exclusion list)
16:26:48.67 -30:35:38.1 -- not an asteroid (will add it to exclusion list)
16:44:25.82 -27:57:21.3 -- asteroid (will NOT add it to exclusion list)
16:02:56.42 -30:30:59.4 -- not an asteroid (will add it to exclusion list)
15:51:27.32 -29:11:13.7 -- not an asteroid (will add it to exclusion list)
16:02:18.75 -20:39:24.8 -- not an asteroid (will add it to exclusion list)
16:53:03.64 -28:34:45.0 -- not an asteroid (will add it to exclusion list)
16:42:57.18 -24:47:27.5 -- not an asteroid (will add it to exclusion list)
15:57:17.70 -20:34:30.5 -- not an asteroid (will add it to exclusion list)
16:53:21.52 -29:12:39.2 -- not an asteroid (will add it to exclusion list)
16:51:46.35 -22:28:38.8 -- not an asteroid (will add it to exclusion list)
16:41:01.72 -29:19:58.1 -- not an asteroid (will add it to exclusion list)
16:04:25.55 -21:17:17.6 -- not an asteroid (will add it to exclusion list)
16:49:25.33 -23:33:25.8 -- not an asteroid (will add it to exclusion list)
16:47:48.94 -27:15:59.9 -- not an asteroid (will add it to exclusion list)
15:52:57.36 -26:39:27.4 -- not an asteroid (will add it to exclusion list)
16:37:29.29 -28:31:54.1 -- not an asteroid (will add it to exclusion list)
16:47:50.31 -29:09:57.8 -- not an asteroid (will add it to exclusion list)
16:40:41.55 -28:09:48.4 -- not an asteroid (will add it to exclusion list)
16:46:02.78 -29:37:25.3 -- not an asteroid (will add it to exclusion list)
16:52:06.26 -21:46:38.3 -- not an asteroid (will add it to exclusion list)
16:29:17.72 -30:22:22.9 -- not an asteroid (will add it to exclusion list)
16:23:57.83 -26:39:21.0 -- not an asteroid (will add it to exclusion list)
15:51:26.26 -26:10:27.4 -- not an asteroid (will add it to exclusion list)
16:03:29.09 -25:11:28.7 -- not an asteroid (will add it to exclusion list)
16:47:27.71 -22:27:42.3 -- not an asteroid (will add it to exclusion list)
16:44:27.44 -29:55:53.7 -- not an asteroid (will add it to exclusion list)
16:48:15.00 -22:44:24.9 -- not an asteroid (will add it to exclusion list)
16:16:10.57 -22:34:12.8 -- not an asteroid (will add it to exclusion list)
16:11:13.63 -22:57:38.0 -- not an asteroid (will add it to exclusion list)
16:02:15.55 -23:17:11.3 -- not an asteroid (will add it to exclusion list)
16:37:29.24 -29:28:54.0 -- not an asteroid (will add it to exclusion list)
16:27:10.14 -29:24:36.9 -- not an asteroid (will add it to exclusion list)
16:48:31.85 -28:45:18.7 -- not an asteroid (will add it to exclusion list)
16:08:00.35 -22:45:34.6 -- not an asteroid (will add it to exclusion list)
16:23:38.71 -25:46:45.4 -- not an asteroid (will add it to exclusion list)
15:52:37.19 -27:42:54.6 -- not an asteroid (will add it to exclusion list)
16:11:06.53 -23:21:07.8 -- not an asteroid (will add it to exclusion list)
16:45:33.93 -29:20:03.5 -- not an asteroid (will add it to exclusion list)
16:32:45.99 -27:17:48.7 -- not an asteroid (will add it to exclusion list)
16:48:41.02 -27:25:00.6 -- not an asteroid (will add it to exclusion list)
15:54:49.55 -30:25:53.0 -- not an asteroid (will add it to exclusion list)
16:19:43.95 -28:59:27.8 -- not an asteroid (will add it to exclusion list)
16:49:20.61 -22:34:12.0 -- not an asteroid (will add it to exclusion list)
16:23:42.53 -29:01:37.0 -- not an asteroid (will add it to exclusion list)
16:09:12.12 -23:36:00.1 -- not an asteroid (will add it to exclusion list)
16:42:45.43 -28:47:47.2 -- not an asteroid (will add it to exclusion list)
16:52:19.47 -22:04:15.8 -- not an asteroid (will add it to exclusion list)
16:03:25.55 -30:38:06.5 -- not an asteroid (will add it to exclusion list)
16:31:27.00 -31:12:46.9 -- not an asteroid (will add it to exclusion list)
15:54:45.72 -25:23:15.7 -- not an asteroid (will add it to exclusion list)
16:39:12.44 -23:29:12.9 -- asteroid (will NOT add it to exclusion list)
16:40:00.12 -30:19:25.5 -- not an asteroid (will add it to exclusion list)
16:35:15.67 -31:07:49.7 -- not an asteroid (will add it to exclusion list)
16:04:35.93 -29:43:24.1 -- not an asteroid (will add it to exclusion list)
16:05:44.05 -25:18:34.0 -- not an asteroid (will add it to exclusion list)
16:03:51.42 -27:36:55.3 -- not an asteroid (will add it to exclusion list)
16:03:53.62 -24:58:59.5 -- not an asteroid (will add it to exclusion list)
15:53:31.90 -29:42:45.0 -- not an asteroid (will add it to exclusion list)
15:46:29.73 -26:29:16.5 -- not an asteroid (will add it to exclusion list)
16:04:21.32 -27:20:11.9 -- not an asteroid (will add it to exclusion list)
16:06:24.31 -26:15:19.6 -- not an asteroid (will add it to exclusion list)
16:36:31.83 -27:21:36.3 -- not an asteroid (will add it to exclusion list)
16:05:19.52 -30:42:03.9 -- not an asteroid (will add it to exclusion list)
16:46:39.40 -23:23:17.9 -- not an asteroid (will add it to exclusion list)
15:50:57.58 -26:09:25.2 -- not an asteroid (will add it to exclusion list)
16:08:06.80 -30:14:48.9 -- not an asteroid (will add it to exclusion list)
15:46:46.05 -24:30:52.3 -- not an asteroid (will add it to exclusion list)
16:23:18.03 -29:53:50.2 -- not an asteroid (will add it to exclusion list)
16:53:26.81 -27:55:55.9 -- not an asteroid (will add it to exclusion list)
16:39:14.70 -30:24:22.5 -- not an asteroid (will add it to exclusion list)
16:02:06.58 -28:54:33.4 -- not an asteroid (will add it to exclusion list)
15:55:38.35 -22:10:59.2 -- not an asteroid (will add it to exclusion list)
16:46:51.02 -29:48:14.8 -- not an asteroid (will add it to exclusion list)
16:47:45.07 -29:51:38.6 -- not an asteroid (will add it to exclusion list)
16:52:39.12 -28:36:07.9 -- not an asteroid (will add it to exclusion list)
16:02:53.02 -26:03:07.8 -- not an asteroid (will add it to exclusion list)
16:12:47.37 -28:44:09.2 -- not an asteroid (will add it to exclusion list)
16:41:59.22 -26:21:43.1 -- not an asteroid (will add it to exclusion list)
16:09:27.83 -30:56:35.4 -- not an asteroid (will add it to exclusion list)
16:45:13.95 -28:20:12.3 -- not an asteroid (will add it to exclusion list)
16:48:47.85 -29:45:44.8 -- not an asteroid (will add it to exclusion list)
16:10:26.11 -20:50:39.5 -- not an asteroid (will add it to exclusion list)
16:50:22.42 -28:32:21.8 -- not an asteroid (will add it to exclusion list)
16:53:13.99 -29:40:47.8 -- not an asteroid (will add it to exclusion list)
16:23:18.46 -30:38:28.6 -- not an asteroid (will add it to exclusion list)
15:52:50.84 -27:25:23.1 -- not an asteroid (will add it to exclusion list)
16:17:37.50 -21:09:37.2 -- not an asteroid (will add it to exclusion list)
16:07:01.00 -28:01:36.6 -- not an asteroid (will add it to exclusion list)
16:47:54.33 -28:09:22.2 -- not an asteroid (will add it to exclusion list)
16:49:08.32 -27:24:44.4 -- not an asteroid (will add it to exclusion list)
15:57:02.17 -28:56:19.7 -- not an asteroid (will add it to exclusion list)
16:46:02.04 -29:43:13.2 -- not an asteroid (will add it to exclusion list)
16:20:04.22 -31:00:51.6 -- not an asteroid (will add it to exclusion list)
16:47:10.20 -26:35:35.8 -- not an asteroid (will add it to exclusion list)
16:53:21.09 -29:48:56.1 -- not an asteroid (will add it to exclusion list)
16:52:26.93 -25:54:30.3 -- not an asteroid (will add it to exclusion list)
16:37:47.70 -27:20:57.3 -- not an asteroid (will add it to exclusion list)
16:27:12.50 -26:01:17.7 -- not an asteroid (will add it to exclusion list)
16:18:31.82 -28:19:39.4 -- not an asteroid (will add it to exclusion list)
15:50:13.62 -29:38:25.4 -- not an asteroid (will add it to exclusion list)
15:58:10.99 -26:58:07.0 -- not an asteroid (will add it to exclusion list)
16:50:11.89 -29:43:30.3 -- not an asteroid (will add it to exclusion list)
16:52:04.59 -28:59:32.4 -- not an asteroid (will add it to exclusion list)
16:48:58.04 -26:27:09.3 -- not an asteroid (will add it to exclusion list)
16:44:13.73 -30:41:33.1 -- not an asteroid (will add it to exclusion list)
16:43:52.90 -25:04:30.3 -- not an asteroid (will add it to exclusion list)
16:42:39.40 -28:55:44.5 -- not an asteroid (will add it to exclusion list)
16:42:12.04 -22:42:16.6 -- not an asteroid (will add it to exclusion list)
16:48:35.39 -28:15:35.4 -- not an asteroid (will add it to exclusion list)
15:50:02.62 -30:25:52.7 -- not an asteroid (will add it to exclusion list)
16:08:06.20 -28:47:29.5 -- not an asteroid (will add it to exclusion list)
16:45:41.11 -28:23:20.4 -- not an asteroid (will add it to exclusion list)
15:52:57.91 -20:46:46.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
15:43:18.82 -28:16:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:30.18 -28:25:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:36.88 -29:14:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:39.68 -28:24:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:54.30 -29:41:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:58.25 -29:32:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:14.24 -29:32:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:38.04 -27:40:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:41.25 -27:55:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:01.24 -30:08:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:05.59 -30:13:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:30.81 -27:58:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:39.43 -27:45:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:40.81 -26:35:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:42.96 -25:44:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:50.62 -27:52:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:09.94 -24:18:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:10.98 -27:36:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:13.78 -28:27:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:19.36 -27:13:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:29.73 -26:29:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:39.49 -24:59:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:46.05 -24:30:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:47.40 -29:27:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:51.53 -28:21:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:51.57 -26:16:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:55.93 -22:16:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:55.16 -29:38:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:12.91 -27:13:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:14.67 -26:10:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:16.61 -28:18:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:59.83 -30:17:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:28.48 -20:31:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:55.52 -29:04:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:57.78 -21:47:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:02.62 -30:25:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:08.82 -23:33:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:13.62 -29:38:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:29.06 -20:40:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:57.58 -26:09:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:26.26 -26:10:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:27.32 -29:11:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:36.48 -28:19:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:36.80 -28:19:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:45.03 -24:49:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:50.92 -20:56:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:52.12 -28:56:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:04.24 -21:11:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:10.68 -25:55:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:37.19 -27:42:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:50.84 -27:25:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:57.36 -26:39:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:57.91 -20:46:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:31.90 -29:42:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:39.16 -27:07:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:45.96 -27:16:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:45.72 -25:23:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:49.55 -30:25:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:55.13 -26:34:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:04.93 -29:58:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:22.15 -22:07:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:38.35 -22:10:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:02.17 -28:56:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:17.70 -20:34:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:29.88 -20:50:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:58:10.99 -26:58:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:07.34 -21:50:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:18.42 -28:49:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:38.31 -21:10:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:01:07.77 -27:36:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:06.58 -28:54:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:15.55 -23:17:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:18.75 -20:39:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:36.33 -26:44:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:53.02 -26:03:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:56.42 -30:30:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:21.30 -28:45:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:25.55 -30:38:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:29.09 -25:11:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:51.42 -27:36:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:53.62 -24:58:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:54.02 -27:40:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:55.67 -24:32:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:21.32 -27:20:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:25.55 -21:17:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:35.93 -29:43:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:05:19.52 -30:42:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:05:44.05 -25:18:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:06:24.31 -26:15:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:01.00 -28:01:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:33.66 -29:41:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:00.35 -22:45:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:03.37 -25:33:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:06.20 -28:47:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:06.80 -30:14:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:18.50 -27:17:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:12.12 -23:36:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:27.83 -30:56:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:46.74 -30:23:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:26.11 -20:50:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:31.99 -29:01:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:11:06.53 -23:21:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:11:13.63 -22:57:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:47.37 -28:44:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:51.65 -24:45:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:13:23.98 -21:58:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:14:22.01 -28:01:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:10.57 -22:34:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:37.50 -21:09:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:18:31.82 -28:19:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:04.53 -29:54:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:12.61 -31:06:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:33.16 -21:55:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:43.95 -28:59:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:48.98 -22:17:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:04.22 -31:00:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:10.73 -27:53:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:15.19 -29:00:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:21.71 -30:51:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:18.03 -29:53:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:18.46 -30:38:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:35.42 -26:31:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:38.71 -25:46:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:42.53 -29:01:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:57.83 -26:39:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:16.94 -31:10:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:48.67 -30:35:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:59.80 -27:55:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:10.14 -29:24:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:12.50 -26:01:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:17.72 -30:22:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:18.30 -30:20:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:30:23.67 -30:05:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:31:27.00 -31:12:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:45.99 -27:17:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:54.17 -28:12:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:15.67 -31:07:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:57.38 -26:49:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:31.83 -27:21:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:05.09 -29:53:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:29.24 -29:28:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:29.29 -28:31:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:47.70 -27:20:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:14.70 -30:24:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:00.12 -30:19:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:41.55 -28:09:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:44.36 -30:29:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:45.38 -31:05:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:01.72 -29:19:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:02.21 -29:19:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:21.66 -30:36:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:41.62 -29:26:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:46.00 -21:12:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:59.22 -26:21:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:59.41 -29:44:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:12.04 -22:42:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:31.49 -24:38:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:39.40 -28:55:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:45.43 -28:47:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:57.18 -24:47:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:06.15 -21:41:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:43.36 -30:45:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:46.69 -25:13:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:51.55 -26:43:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:52.90 -25:04:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:00.37 -25:29:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:02.37 -26:58:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:13.73 -30:41:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:17.45 -22:06:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:19.94 -26:19:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:27.44 -29:55:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:28.32 -29:55:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:40.05 -30:23:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:13.95 -28:20:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:24.16 -28:31:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:26.17 -30:58:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:33.93 -29:20:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:41.11 -28:23:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:45.70 -28:50:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:02.04 -29:43:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:02.78 -29:37:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:11.08 -29:29:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:13.27 -29:46:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:15.66 -29:09:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:39.40 -23:23:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:43.92 -24:52:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:51.02 -29:48:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:04.30 -25:48:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:04.94 -25:48:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:08.97 -31:11:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:10.20 -26:35:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:25.37 -23:58:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:27.34 -22:08:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:27.71 -22:27:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:45.07 -29:51:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:45.23 -27:37:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:48.94 -27:15:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:50.31 -29:09:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:53.49 -29:45:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:53.69 -31:06:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:54.33 -28:09:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:00.38 -28:53:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:12.82 -23:20:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:15.00 -22:44:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:22.23 -26:05:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:31.85 -28:45:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:33.49 -25:50:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:35.39 -28:15:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:36.21 -26:02:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:41.02 -27:25:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:47.85 -29:45:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:52.24 -28:26:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:58.04 -26:27:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:58.07 -26:13:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:04.81 -28:14:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:06.33 -22:48:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:07.29 -23:11:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:08.32 -27:24:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:18.35 -28:02:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:20.61 -22:34:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:25.33 -23:33:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:29.05 -31:04:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:37.84 -30:24:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:47.56 -27:33:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:58.85 -30:38:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:11.89 -29:43:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:22.42 -28:32:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:23.00 -28:32:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:44.80 -30:18:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:46.59 -30:07:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:53.23 -23:28:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:19.97 -28:39:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:29.02 -29:05:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:35.56 -29:55:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:37.18 -24:47:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:43.72 -23:54:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:46.35 -22:28:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:47.43 -25:38:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:59.48 -21:28:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:00.63 -28:00:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:04.59 -28:59:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:06.26 -21:46:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:08.21 -28:08:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:09.48 -28:12:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:19.47 -22:04:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:23.89 -23:34:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:26.93 -25:54:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:33.24 -29:17:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:34.37 -30:39:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:39.12 -28:36:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:43.50 -24:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:44.92 -26:36:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:48.67 -30:36:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:50.90 -29:00:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:00.82 -27:34:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:01.49 -30:12:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:03.64 -28:34:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:05.25 -30:38:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:10.74 -29:07:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:13.99 -29:40:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:14.38 -29:31:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:16.51 -28:44:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:21.09 -29:48:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:21.52 -29:12:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:22.02 -29:43:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:25.16 -29:56:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:26.81 -27:55:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:43.51 -23:13:04.7 -- 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)
15:43:18.82 -28:16:54.0 -- not a known variable star
15:43:30.18 -28:25:13.8 -- not a known variable star
15:43:36.88 -29:14:38.9 -- not a known variable star
15:43:39.68 -28:24:04.2 -- not a known variable star
15:43:54.30 -29:41:30.0 -- not a known variable star
15:43:58.25 -29:32:18.2 -- not a known variable star
15:44:14.24 -29:32:00.7 -- not a known variable star
15:44:38.04 -27:40:12.7 -- a known variable star
15:44:41.25 -27:55:43.5 -- not a known variable star
15:45:01.24 -30:08:11.0 -- not a known variable star
15:45:05.59 -30:13:20.0 -- not a known variable star
15:45:30.81 -27:58:17.5 -- not a known variable star
15:45:39.43 -27:45:33.0 -- not a known variable star
15:45:40.81 -26:35:12.7 -- not a known variable star
15:45:42.96 -25:44:31.8 -- a known variable star
15:45:50.62 -27:52:55.7 -- not a known variable star
15:46:09.94 -24:18:31.5 -- not a known variable star
15:46:10.98 -27:36:48.3 -- a known variable star
15:46:13.78 -28:27:49.6 -- not a known variable star
15:46:19.36 -27:13:15.2 -- not a known variable star
15:46:29.73 -26:29:16.5 -- not a known variable star
15:46:39.49 -24:59:09.5 -- not a known variable star
15:46:46.05 -24:30:52.3 -- not a known variable star
15:46:47.40 -29:27:31.4 -- not a known variable star
15:46:51.53 -28:21:55.7 -- not a known variable star
15:46:51.57 -26:16:15.4 -- not a known variable star
15:46:55.93 -22:16:18.4 -- a known variable star
15:47:55.16 -29:38:04.8 -- a known variable star
15:48:12.91 -27:13:12.5 -- not a known variable star
15:48:14.67 -26:10:25.1 -- not a known variable star
15:48:16.61 -28:18:27.1 -- not a known variable star
15:48:59.83 -30:17:18.3 -- not a known variable star
15:49:28.48 -20:31:27.2 -- not a known variable star
15:49:55.52 -29:04:17.7 -- not a known variable star
15:49:57.78 -21:47:19.5 -- not a known variable star
15:50:02.62 -30:25:52.7 -- not a known variable star
15:50:08.82 -23:33:23.1 -- a known variable star
15:50:13.62 -29:38:25.4 -- a known variable star
15:50:29.06 -20:40:25.1 -- not a known variable star
15:50:57.58 -26:09:25.2 -- not a known variable star
15:51:26.26 -26:10:27.4 -- a known variable star
15:51:27.32 -29:11:13.7 -- not a known variable star
15:51:36.48 -28:19:08.1 -- not a known variable star
15:51:36.80 -28:19:11.0 -- not a known variable star
15:51:45.03 -24:49:27.3 -- not a known variable star
15:51:50.92 -20:56:52.8 -- not a known variable star
15:51:52.12 -28:56:49.5 -- not a known variable star
15:52:04.24 -21:11:00.5 -- not a known variable star
15:52:10.68 -25:55:30.2 -- not a known variable star
15:52:37.19 -27:42:54.6 -- not a known variable star
15:52:50.84 -27:25:23.1 -- not a known variable star
15:52:57.36 -26:39:27.4 -- not a known variable star
15:52:57.91 -20:46:46.8 -- not a known variable star
15:53:31.90 -29:42:45.0 -- not a known variable star
15:53:39.16 -27:07:15.0 -- a known variable star
15:53:45.96 -27:16:25.9 -- a known variable star
15:54:45.72 -25:23:15.7 -- not a known variable star
15:54:49.55 -30:25:53.0 -- not a known variable star
15:54:55.13 -26:34:47.9 -- not a known variable star
15:55:04.93 -29:58:22.7 -- not a known variable star
15:55:22.15 -22:07:22.9 -- not a known variable star
15:55:38.35 -22:10:59.2 -- a known variable star
15:57:02.17 -28:56:19.7 -- a known variable star
15:57:17.70 -20:34:30.5 -- not a known variable star
15:57:29.88 -20:50:56.5 -- not a known variable star
15:58:10.99 -26:58:07.0 -- a known variable star
15:59:07.34 -21:50:41.4 -- a known variable star
15:59:18.42 -28:49:45.9 -- not a known variable star
15:59:38.31 -21:10:43.1 -- a known variable star
16:01:07.77 -27:36:07.1 -- not a known variable star
16:02:06.58 -28:54:33.4 -- not a known variable star
16:02:15.55 -23:17:11.3 -- not a known variable star
16:02:18.75 -20:39:24.8 -- not a known variable star
16:02:36.33 -26:44:13.5 -- a known variable star
16:02:53.02 -26:03:07.8 -- not a known variable star
16:02:56.42 -30:30:59.4 -- not a known variable star
16:03:21.30 -28:45:09.6 -- not a known variable star
16:03:25.55 -30:38:06.5 -- not a known variable star
16:03:29.09 -25:11:28.7 -- a known variable star
16:03:51.42 -27:36:55.3 -- not a known variable star
16:03:53.62 -24:58:59.5 -- not a known variable star
16:03:54.02 -27:40:31.8 -- not a known variable star
16:03:55.67 -24:32:35.8 -- not a known variable star
16:04:21.32 -27:20:11.9 -- not a known variable star
16:04:25.55 -21:17:17.6 -- not a known variable star
16:04:35.93 -29:43:24.1 -- not a known variable star
16:05:19.52 -30:42:03.9 -- a known variable star
16:05:44.05 -25:18:34.0 -- not a known variable star
16:06:24.31 -26:15:19.6 -- not a known variable star
16:07:01.00 -28:01:36.6 -- not a known variable star
16:07:33.66 -29:41:13.3 -- a known variable star
16:08:00.35 -22:45:34.6 -- not a known variable star
16:08:03.37 -25:33:07.6 -- not a known variable star
16:08:06.20 -28:47:29.5 -- not a known variable star
16:08:06.80 -30:14:48.9 -- not a known variable star
16:08:18.50 -27:17:11.6 -- a known variable star
16:09:12.12 -23:36:00.1 -- not a known variable star
16:09:27.83 -30:56:35.4 -- not a known variable star
16:09:46.74 -30:23:54.2 -- not a known variable star
16:10:26.11 -20:50:39.5 -- not a known variable star
16:10:31.99 -29:01:39.8 -- a known variable star
16:11:06.53 -23:21:07.8 -- not a known variable star
16:11:13.63 -22:57:38.0 -- a known variable star
16:12:47.37 -28:44:09.2 -- not a known variable star
16:12:51.65 -24:45:29.1 -- not a known variable star
16:13:23.98 -21:58:10.0 -- not a known variable star
16:14:22.01 -28:01:16.5 -- not a known variable star
16:16:10.57 -22:34:12.8 -- a known variable star
16:17:37.50 -21:09:37.2 -- not a known variable star
16:18:31.82 -28:19:39.4 -- a known variable star
16:19:04.53 -29:54:16.3 -- not a known variable star
16:19:12.61 -31:06:40.6 -- not a known variable star
16:19:33.16 -21:55:41.3 -- not a known variable star
16:19:43.95 -28:59:27.8 -- not a known variable star
16:19:48.98 -22:17:37.1 -- a known variable star
16:20:04.22 -31:00:51.6 -- not a known variable star
16:21:10.73 -27:53:04.1 -- not a known variable star
16:21:15.19 -29:00:33.2 -- not a known variable star
16:22:21.71 -30:51:17.2 -- a known variable star
16:23:18.03 -29:53:50.2 -- a known variable star
16:23:18.46 -30:38:28.6 -- a known variable star
16:23:35.42 -26:31:37.7 -- a known variable star
16:23:38.71 -25:46:45.4 -- not a known variable star
16:23:42.53 -29:01:37.0 -- not a known variable star
16:23:57.83 -26:39:21.0 -- not a known variable star
16:24:16.94 -31:10:22.5 -- not a known variable star
16:26:48.67 -30:35:38.1 -- not a known variable star
16:26:59.80 -27:55:10.7 -- not a known variable star
16:27:10.14 -29:24:36.9 -- not a known variable star
16:27:12.50 -26:01:17.7 -- not a known variable star
16:29:17.72 -30:22:22.9 -- not a known variable star
16:29:18.30 -30:20:41.8 -- not a known variable star
16:30:23.67 -30:05:02.0 -- not a known variable star
16:31:27.00 -31:12:46.9 -- not a known variable star
16:32:45.99 -27:17:48.7 -- a known variable star
16:33:54.17 -28:12:42.4 -- not a known variable star
16:35:15.67 -31:07:49.7 -- not a known variable star
16:35:57.38 -26:49:34.8 -- not a known variable star
16:36:31.83 -27:21:36.3 -- not a known variable star
16:37:05.09 -29:53:35.5 -- not a known variable star
16:37:29.24 -29:28:54.0 -- not a known variable star
16:37:29.29 -28:31:54.1 -- a known variable star
16:37:47.70 -27:20:57.3 -- a known variable star
16:39:14.70 -30:24:22.5 -- a known variable star
16:40:00.12 -30:19:25.5 -- a known variable star
16:40:41.55 -28:09:48.4 -- not a known variable star
16:40:44.36 -30:29:38.4 -- not a known variable star
16:40:45.38 -31:05:31.7 -- not a known variable star
16:41:01.72 -29:19:58.1 -- not a known variable star
16:41:02.21 -29:19:48.1 -- not a known variable star
16:41:21.66 -30:36:21.7 -- not a known variable star
16:41:41.62 -29:26:40.2 -- not a known variable star
16:41:46.00 -21:12:43.8 -- not a known variable star
16:41:59.22 -26:21:43.1 -- not a known variable star
16:41:59.41 -29:44:48.6 -- not a known variable star
16:42:12.04 -22:42:16.6 -- a known variable star
16:42:31.49 -24:38:08.6 -- not a known variable star
16:42:39.40 -28:55:44.5 -- a known variable star
16:42:45.43 -28:47:47.2 -- not a known variable star
16:42:57.18 -24:47:27.5 -- not a known variable star
16:43:06.15 -21:41:24.0 -- not a known variable star
16:43:43.36 -30:45:03.1 -- not a known variable star
16:43:46.69 -25:13:32.6 -- not a known variable star
16:43:51.55 -26:43:04.5 -- not a known variable star
16:43:52.90 -25:04:30.3 -- not a known variable star
16:44:00.37 -25:29:57.9 -- not a known variable star
16:44:02.37 -26:58:20.4 -- not a known variable star
16:44:13.73 -30:41:33.1 -- not a known variable star
16:44:17.45 -22:06:53.4 -- a known variable star
16:44:19.94 -26:19:30.5 -- not a known variable star
16:44:27.44 -29:55:53.7 -- a known variable star
16:44:28.32 -29:55:23.4 -- not a known variable star
16:44:40.05 -30:23:22.3 -- a known variable star
16:45:13.95 -28:20:12.3 -- not a known variable star
16:45:24.16 -28:31:44.6 -- not a known variable star
16:45:26.17 -30:58:52.3 -- a known variable star
16:45:33.93 -29:20:03.5 -- not a known variable star
16:45:41.11 -28:23:20.4 -- not a known variable star
16:45:45.70 -28:50:38.2 -- not a known variable star
16:46:02.04 -29:43:13.2 -- a known variable star
16:46:02.78 -29:37:25.3 -- not a known variable star
16:46:11.08 -29:29:15.5 -- a known variable star
16:46:13.27 -29:46:18.6 -- not a known variable star
16:46:15.66 -29:09:41.6 -- not a known variable star
16:46:39.40 -23:23:17.9 -- not a known variable star
16:46:43.92 -24:52:08.8 -- not a known variable star
16:46:51.02 -29:48:14.8 -- a known variable star
16:47:04.30 -25:48:40.7 -- not a known variable star
16:47:04.94 -25:48:42.3 -- a known variable star
16:47:08.97 -31:11:01.8 -- a known variable star
16:47:10.20 -26:35:35.8 -- not a known variable star
16:47:25.37 -23:58:16.2 -- a known variable star
16:47:27.34 -22:08:47.5 -- not a known variable star
16:47:27.71 -22:27:42.3 -- not a known variable star
16:47:45.07 -29:51:38.6 -- not a known variable star
16:47:45.23 -27:37:40.7 -- not a known variable star
16:47:48.94 -27:15:59.9 -- not a known variable star
16:47:50.31 -29:09:57.8 -- not a known variable star
16:47:53.49 -29:45:24.3 -- not a known variable star
16:47:53.69 -31:06:09.7 -- a known variable star
16:47:54.33 -28:09:22.2 -- a known variable star
16:48:00.38 -28:53:32.6 -- a known variable star
16:48:12.82 -23:20:44.7 -- not a known variable star
16:48:15.00 -22:44:24.9 -- not a known variable star
16:48:22.23 -26:05:37.2 -- not a known variable star
16:48:31.85 -28:45:18.7 -- not a known variable star
16:48:33.49 -25:50:33.8 -- not a known variable star
16:48:35.39 -28:15:35.4 -- not a known variable star
16:48:36.21 -26:02:22.2 -- not a known variable star
16:48:41.02 -27:25:00.6 -- a known variable star
16:48:47.85 -29:45:44.8 -- not a known variable star
16:48:52.24 -28:26:08.4 -- not a known variable star
16:48:58.04 -26:27:09.3 -- not a known variable star
16:48:58.07 -26:13:47.0 -- not a known variable star
16:49:04.81 -28:14:44.5 -- not a known variable star
16:49:06.33 -22:48:55.9 -- not a known variable star
16:49:07.29 -23:11:32.6 -- a known variable star
16:49:08.32 -27:24:44.4 -- a known variable star
16:49:18.35 -28:02:13.2 -- not a known variable star
16:49:20.61 -22:34:12.0 -- not a known variable star
16:49:25.33 -23:33:25.8 -- a known variable star
16:49:29.05 -31:04:15.9 -- not a known variable star
16:49:37.84 -30:24:59.8 -- not a known variable star
16:49:47.56 -27:33:22.5 -- not a known variable star
16:49:58.85 -30:38:19.6 -- not a known variable star
16:50:11.89 -29:43:30.3 -- not a known variable star
16:50:22.42 -28:32:21.8 -- not a known variable star
16:50:23.00 -28:32:20.9 -- not a known variable star
16:50:44.80 -30:18:17.4 -- not a known variable star
16:50:46.59 -30:07:55.5 -- a known variable star
16:50:53.23 -23:28:24.0 -- not a known variable star
16:51:19.97 -28:39:28.8 -- not a known variable star
16:51:29.02 -29:05:27.9 -- not a known variable star
16:51:35.56 -29:55:38.1 -- not a known variable star
16:51:37.18 -24:47:58.2 -- not a known variable star
16:51:43.72 -23:54:10.9 -- not a known variable star
16:51:46.35 -22:28:38.8 -- not a known variable star
16:51:47.43 -25:38:14.9 -- a known variable star
16:51:59.48 -21:28:54.4 -- not a known variable star
16:52:00.63 -28:00:49.6 -- not a known variable star
16:52:04.59 -28:59:32.4 -- a known variable star
16:52:06.26 -21:46:38.3 -- not a known variable star
16:52:08.21 -28:08:52.9 -- not a known variable star
16:52:09.48 -28:12:42.5 -- not a known variable star
16:52:19.47 -22:04:15.8 -- not a known variable star
16:52:23.89 -23:34:13.5 -- a known variable star
16:52:26.93 -25:54:30.3 -- not a known variable star
16:52:33.24 -29:17:25.9 -- not a known variable star
16:52:34.37 -30:39:27.7 -- a known variable star
16:52:39.12 -28:36:07.9 -- not a known variable star
16:52:43.50 -24:26:08.0 -- a known variable star
16:52:44.92 -26:36:39.6 -- not a known variable star
16:52:48.67 -30:36:24.1 -- not a known variable star
16:52:50.90 -29:00:02.0 -- not a known variable star
16:53:00.82 -27:34:28.6 -- not a known variable star
16:53:01.49 -30:12:02.9 -- not a known variable star
16:53:03.64 -28:34:45.0 -- not a known variable star
16:53:05.25 -30:38:15.9 -- not a known variable star
16:53:10.74 -29:07:44.7 -- a known variable star
16:53:13.99 -29:40:47.8 -- not a known variable star
16:53:14.38 -29:31:09.5 -- not a known variable star
16:53:16.51 -28:44:26.9 -- not a known variable star
16:53:21.09 -29:48:56.1 -- not a known variable star
16:53:21.52 -29:12:39.2 -- not a known variable star
16:53:22.02 -29:43:16.9 -- not a known variable star
16:53:25.16 -29:56:29.4 -- not a known variable star
16:53:26.81 -27:55:55.9 -- not a known variable star
16:53:43.51 -23:13:04.7 -- a known variable star
Found 207 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
268 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 268 (excluding asteroids and hot pixels, 207 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)2461150.92438853 -observatory V36
00:31:36.65 +00:33:57.2 Mercury (-0.1mag)
03:30:28.07 +19:26:15.5 Venus (-3.9mag)
00:30:23.96 +02:14:32.6 Mars (1.2mag)
07:14:44.63 +22:42:41.1 Jupiter (-2.1mag)
00:31:08.33 +01:01:07.9 Saturn (0.9mag)
03:48:38.73 +19:50:29.9 Uranus (5.8mag)
00:11:24.68 -00:11:47.1 Neptune (7.8mag)
20:33:55.75 -22:52:52.5 Pluto (14.5mag)
04:33:54.43 +26:13:55.8 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 362 Apr 20 05:14 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461150.92438853:
07:14:46.96 +22:42:33.6 Io (5.8mag)
07:14:57.10 +22:42:13.3 Europa (5.9mag)
07:14:37.86 +22:43:02.1 Ganymede (5.4mag)
07:14:44.49 +22:42:31.9 Callisto (6.6mag)
07:17:52.64 +22:28:20.1 Himalia (15.4mag)
07:14:44.29 +22:42:44.0 Thebe (16.3mag)
07:18:09.35 +22:58:40.3 Elara (17.3mag)
07:13:55.58 +23:20:22.5 Pasiphae (17.4mag)
07:22:58.22 +22:41:07.0 Carme (18.5mag)
00:30:59.01 +01:01:20.9 Titan (8.8mag)
00:31:05.78 +01:01:14.2 Rhea (10.1mag)
00:30:42.07 +01:00:34.9 Iapetus (11.5mag)
00:31:00.31 +01:01:33.3 Hyperion (14.8mag)
00:32:41.60 +01:09:26.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 20 05:14 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461150.92438853:
15:55:30.61 -19:13:42.2 JWST
18:31:48.21 +27:04:00.0 Chandra
09:02:41.87 -51:31:11.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 20 05:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461150.92438853 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:35.52 -29:02:48.8 13.9mag P/2010 H2 (Vales)
05:10:00.01 -69:27:29.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:27.44 +31:28:07.4 17.2mag C/2017 K2 (PANSTARRS)
17:29:53.73 +11:03:56.1 17.6mag C/2021 G2 (ATLAS)
23:11:19.76 +29:24:36.3 17.1mag C/2022 E2 (ATLAS)
04:34:26.06 +26:09:20.3 16.1mag C/2022 N2 (PANSTARRS)
09:04:30.08 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:31:51.24 +00:18:14.2 17.4mag C/2022 R6 (PANSTARRS)
18:52:33.97 +18:53:53.8 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:09.95 -11:27:23.0 17.5mag P/2023 B1 (PANSTARRS)
09:05:44.83 -11:11:20.9 17.7mag C/2023 F3 (ATLAS)
21:58:25.82 +63:10:28.6 17.5mag C/2023 H5 (Lemmon)
19:15:02.35 -03:49:00.3 14.1mag C/2023 R1 (PANSTARRS)
21:20:01.01 +86:31:58.3 17.8mag C/2023 X2 (Lemmon)
06:20:13.99 +63:30:01.8 17.2mag C/2024 A1 (ATLAS)
05:22:32.26 +19:40:55.7 11.3mag C/2024 E1 (Wierzchos)
16:16:19.22 +07:06:40.8 17.3mag C/2024 G6 (ATLAS)
20:21:54.66 +16:29:36.9 14.5mag C/2024 J3 (ATLAS)
03:30:23.40 -21:43:26.6 16.3mag C/2024 T5 (ATLAS)
05:20:32.00 +44:13:04.3 17.7mag C/2025 J1 (Borisov)
13:20:41.90 +48:00:13.6 15.4mag C/2025 L1 (ATLAS)
03:32:25.50 -26:55:18.1 17.9mag C/2025 Q3 (ATLAS)
00:36:02.34 +16:01:43.7 8.0mag C/2025 R3 (PANSTARRS)
12:52:13.45 +03:16:23.6 17.4mag C/2025 Y1 (ATLAS)
03:59:39.12 +02:14:24.9 14.5mag C/2026 A1 (MAPS)
00:11:53.51 +37:59:44.4 14.7mag C/2026 B2 (Sun-Gao)
18:51:31.68 -09:28:43.9 11.6mag 10P/Tempel
14:54:15.20 +02:43:06.2 14.4mag 24P/Schaumasse
11:01:42.89 -01:23:25.5 15.7mag 29P/Schwassmann-Wachmann
10:37:36.75 -03:46:05.8 17.0mag 43P/Wolf-Harrington
01:55:32.42 +18:14:08.3 17.3mag 47P/Ashbrook-Jackson
07:19:04.93 +36:02:58.1 17.0mag 63P/Wild
23:34:38.13 -10:55:38.6 15.7mag 65P/Gunn
04:15:14.58 +22:44:03.6 15.9mag 76P/West-Kohoutek-Ikemura
01:15:24.79 +09:05:31.0 14.3mag 78P/Gehrels
23:16:12.67 -08:04:56.3 14.7mag 88P/Howell
02:23:03.94 +21:47:47.9 15.1mag 93P/Lovas
05:03:18.08 +32:30:42.5 16.1mag 123P/West-Hartley
08:33:48.93 +36:19:20.5 16.2mag 124P/Mrkos
02:40:05.84 +14:51:26.3 16.4mag 128P/Shoemaker-Holt
02:56:14.87 +15:01:12.5 17.5mag 131P/Mueller
01:49:40.85 +14:41:12.1 10.5mag 141P/Machholz
01:57:54.91 +06:31:10.9 10.5mag 141P-A/Machholz
00:41:16.68 +02:18:15.8 12.3mag 141P-D/Machholz
02:28:29.77 +08:16:09.1 17.9mag 141P-I/Machholz
01:14:46.24 +00:42:25.5 15.0mag 162P/SidingSpring
14:43:37.25 +00:21:06.7 17.8mag 210P/Christensen
21:51:15.78 -10:23:26.7 17.7mag 218P/LINEAR
17:17:17.33 -13:23:41.6 16.1mag 235P/LINEAR
05:44:07.60 +35:00:26.1 16.8mag 240P/NEAT
07:40:47.95 -04:42:15.7 17.8mag 242P/Spahr
22:27:58.96 -19:46:08.9 17.8mag 260P/McNaught
02:07:19.95 +21:34:00.4 18.0mag 295P/LINEAR
15:40:47.96 +07:16:12.2 17.5mag 391P/Kowalski
07:36:01.03 +21:22:23.3 17.7mag 450P/LONEOS
05:42:24.76 +44:46:26.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 20 05:14 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 05:14 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 05:14 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 05:14 tns_transients_list.txt
